The galaxy appears as an elliptical or lenticular type. Its shape is elongated, with a noticeable cigar-like appearance. The central bulge exhibits a bright, smooth, and concentrated distribution of light, suggestive of an older stellar population. Progressing outwards from the core, the light gradually diminishes with no apparent spiral arm structure. The color gradient shifts from a yellowish hue in the center to a bluer tone at the edges, indicating regions of more recent star formation towards the outer parts of the galaxy. There are no prominent tidal features or signs of major ongoing mergers, although subtle asymmetries hint at possible past interactions. Overall, this galaxy presents as a relatively undisturbed system dominated by older stars, but with some evidence of more recent star formation in the outer regions.
