This galaxy presents an elliptical morphology, appearing smooth and somewhat elongated in shape. The central region displays a concentrated luminosity, gradually diminishing outwards. The color profile suggests a predominantly older stellar population, exhibiting a yellowish-red hue. There are some indications of minor disturbances in its structure, possibly due to interactions with smaller companions or past merger events. However, it does not seem to be currently undergoing a major merging event. There is a lack of any clear spiral arm structure, further supporting its classification as an elliptical galaxy. 
