The galaxy appears as a centrally concentrated, elliptical structure with a smooth, diffuse profile. There is no clear evidence of spiral arms or a distinct disk component. The central region exhibits a bright, compact core, suggesting a high concentration of stars or an active galactic nucleus (AGN), though the resolution of the image limits definitive identification. The galaxy's overall color appears to be relatively uniform, exhibiting a yellowish-white hue, indicating a stellar population dominated by older, less massive stars. There is no immediately obvious evidence of ongoing major star formation, nor any substantial dust lanes. The morphology of the galaxy suggests it is likely an early-type galaxy, specifically an elliptical galaxy, with a round shape and a generally smooth texture. There are no noticeable tidal tails or other indicators of recent or ongoing merger activity.
