The galaxy presents an overall elliptical morphology, appearing largely smooth with a concentrated central bulge. The color profile suggests a relatively older stellar population, with a general redder hue. There may be limited star formation activity, based on the lack of distinct blue regions. The galaxy exhibits some degree of asymmetry in its outer regions, possibly indicating a past or ongoing minor interaction or disturbance. The light distribution is generally diffuse, showing a gradual decrease in brightness moving outward from the core. The overall rounded appearance suggests the galaxy is relatively relaxed and not undergoing a major merger event.
