The galaxy presents a generally smooth, elongated morphology, exhibiting a prolate spheroid shape. It's major axis appears to be significantly longer than it's minor axis. The central region demonstrates a higher surface brightness, suggesting a dense stellar population, or possibly a small active galactic nucleus, but this can not be confirmed from the image alone. The outer regions of the galaxy fade gradually, indicating a diffuse halo or extended stellar envelope.

There are faint, subtle color gradients across the galaxy, with the central region appearing somewhat yellower compared to the bluer outer edges. This could be suggestive of differential stellar populations, with older, redder stars concentrated in the core and younger, bluer stars residing in the outer regions where star formation may still be occurring. There's no discernible spiral structure, distinct dust lanes, or significant tidal features visible in the image. The lack of any major disturbances could imply the galaxy is in relative isolation. No signs of on going mergers are apparent from the image, although there are a few disturbances that are apparent.
