The galaxy appears to be a relatively smooth, elliptical or lenticular type. It displays a bright central bulge, possibly an active galactic nucleus, surrounded by a more diffuse halo of stars. There is little evidence of spiral arms or dust lanes. The galaxy exhibits a slight elongation in its morphology, deviating from a perfectly circular shape. There are no major signs of tidal disturbances or ongoing mergers, suggesting a relatively quiescent evolutionary state. The color distribution is fairly uniform, implying a lack of significant recent star formation activity. The galaxy seems dominated by an older stellar population. Overall, it presents a classic morphology of an evolved galaxy.
