The galaxy appears as a somewhat flattened elliptical or lenticular system, presenting a smooth and diffuse profile with an absence of distinct spiral arms. The central bulge is bright and concentrated, exhibiting a yellowish-white hue. This suggests a population of older, less massive stars. The outer regions show a gradual decrease in luminosity and appear slightly bluer, hinting at the presence of some younger stellar populations and ongoing star formation. There appears to be only a slight dust lane, indicating that this is probably a well settled system that isn't undergoing major changes. The system shows an estimated mass to be quite high, suggesting that it is quite a massive system. Overall, the galaxy appears to be in a relatively settled state, displaying characteristics intermediate between elliptical and spiral morphologies.