The galaxy presents an elliptical morphology, appearing somewhat flattened. Its color profile is predominantly bluish, suggesting the presence of a younger stellar population and ongoing star formation activity. There is a central bulge region, characterized by a higher concentration of light, from which the luminosity gradually decreases towards the outer edges of the galaxy. The smooth light distribution implies a relatively homogenous stellar population with no discernible spiral arm structure or distinct features indicating active galactic nuclei activity.
