The galaxy presents a somewhat elliptical morphology, appearing largely smooth and relatively concentrated. A bright central bulge is visible, exhibiting a yellowish-orange hue, potentially indicating an older stellar population. Surrounding the bulge is a less defined disk, exhibiting a mix of colors, including some regions with a greenish-blue tint. This suggests ongoing or recent star formation activity within the disk component. There are several distinct, concentrated points of light outside the central bulge, perhaps indicating localized star formation. The overall structure displays some evidence of minor disturbances, with a hint of asymmetry in the outer regions. There is the possibility of recent or ongoing interaction. The relatively smooth appearance and concentrated light distribution suggest it could be an early-type spiral or a lenticular galaxy.
