The galaxy presents as an elliptical or lenticular type, with a smooth, concentrated central bulge. The bulge appears yellowish, possibly indicating an older stellar population. There's a slight elongation in the galaxy's shape, suggesting it is not perfectly spherical but more likely an oblate spheroid. The outer regions fade gradually into the background, with a lower surface brightness compared to the bulge. There is evidence of some faint features to the south, possibly indicating a disk-like component or a region of increased star formation. There does not appear to be a clear, prominent disk or spiral arm structure, nor is there any indication of ongoing major merging activity or significant tidal disturbances.
