The galaxy presents as a moderately concentrated object with a primarily smooth morphology, exhibiting a bright central region indicative of a bulge. The overall shape appears somewhat rounded, but not perfectly spherical. There is a slight elongation noticeable, suggesting it may be transitioning away from a purely elliptical form. The color is predominantly yellow and red, suggesting a population of older stars and a relatively low rate of ongoing star formation. There may be some minor disturbances or asymmetries visible, but they are subtle and do not indicate a major ongoing merger event. It's possible there has been a small tidal interaction in the past that has left some minor disruption in the shape of the galaxy.
