The galaxy presents a largely smooth and elliptical morphology. Its central region exhibits a bright, concentrated core, indicative of a possible active galactic nucleus or a dense stellar population. The light distribution gradually fades outward from the center, suggesting a relatively old stellar population dominating the overall structure. There is a subtle extension visible in the galaxy's shape, hinting at a minor deviation from perfect ellipticity. This might be the result of a past or ongoing interaction, although no distinct tidal features or strong signs of a merger are immediately apparent in this image. The color appears to be fairly uniform across the galaxy, indicating similar stellar populations.
