The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density, with colors that appear to be in the yellow to white range. The light suggests an older stellar population. Moving outward, the galaxy gradually fades, displaying a smoother profile with decreasing surface brightness. The colors shift slightly to redder hues, indicating the possible presence of older stars or dust. There are no discernible spiral arms or distinct features in the galaxy disk, reinforcing its classification as an elliptical galaxy. The overall impression is one of a relatively quiescent galaxy, not actively undergoing significant star formation, but with a low level of it ongoing. There is no clear indication of any major merger events or significant disturbances in its structure, although there might be very subtle, minor disturbances present.
