The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a dominant central bulge and a relatively smooth disk. There is a yellowish-white glow suggesting an older stellar population and minimal active star formation, concentrated towards the nucleus. The galaxy has a slight elongation. No distinct spiral arm structure is discernible. There are no significant signs of tidal interactions or ongoing mergers. There are some hints of faint, dusty features within the disk. The object generally shows a well-ordered, stable structure with minimal disturbances.
