The galaxy presents as a centrally concentrated elliptical type, exhibiting a smooth, diffuse morphology. The overall color profile appears relatively uniform, tending toward a yellowish-white hue, suggestive of an older stellar population dominating the light emission. The light distribution is consistent with a relatively spherical or slightly elongated shape with no clear evidence of spiral arms or a prominent disk. There are no obvious signs of active galactic nuclei activity or significant dust lanes visible in the image. Faint extensions or tidal features are not immediately apparent, suggesting a galaxy that is not currently undergoing a major merger event. The apparent lack of distinct features may indicate a quiescent state, possibly past its peak star-forming period.
