The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the edges. A distinct, brighter, more compact region is observed near the galaxy's bottom section. This could be a sign of disturbance or a merger. The galaxy's light profile is relatively smooth with no distinct spiral arm structures visible. The color appears yellowish and potentially old. Overall, the galaxy appears to be relatively massive and possibly in the later stages of its evolution.
