The galaxy presents as a centrally concentrated object, exhibiting a generally smooth and rounded morphology. There is little evidence of significant spiral arm structure or a distinct bar. A slight ellipticity is observable, but the galaxy appears close to circular when viewed face-on. A faint disk is faintly visible.

The galaxy's color profile is primarily homogenous, indicating a relatively uniform stellar population. The central region appears marginally brighter, suggesting a higher stellar density or the presence of an active galactic nucleus (AGN), though this is not distinctly discernible from the image alone. There are no prominent dust lanes or patches visible, indicating the lack of significant dust obscuration. A few minor disturbances can be seen in the galaxy, but appear to be generally small and do not disrupt the overall galaxy. The outer regions of the galaxy gradually fade into the background sky, with no clear demarcation of a stellar halo.

The overall impression is that of a lenticular or early-type spiral galaxy, possibly undergoing relatively quiescent star formation.
