The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggestive of a significant stellar population and potentially, an active galactic nucleus. There is an area of redder hue on the outskirt of the core, suggesting some more recent star forming areas. While the main structure is quite well defined, there's a subtle irregularity or minor disturbance visible on one edge. This could be due to an ongoing or past merger event, or perhaps interactions with smaller satellite galaxies. The overall light profile fades gradually from the core outwards, indicating a relatively old and evolved stellar population dominating the outer regions, consistent with an elliptical galaxy type. 
