The galaxy appears as a moderately bright, lenticular object with a dominant central bulge. Its light is notably concentrated toward the core, which exhibits a smooth, elliptical morphology. While some asymmetry is present, the galaxy lacks any distinct spiral arm structure or prominent dust lanes. The general color is fairly consistent with a lack of patchiness, suggesting an older stellar population. There is some possible minor disruption within the system that could point to an ongoing or recent minor merger event.
