The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The light distribution suggests a morphology that leans toward elliptical, exhibiting a high degree of central concentration. There are no visually discernible spiral arms or prominent dust lanes. The color is generally yellowish-white, indicating a stellar population dominated by older stars, but there are faint blueish hints. There isn't strong evidence of ongoing star formation, as might be indicated by bluer regions. The shape appears nearly circular, exhibiting little ellipticity, indicating its type to be closest to an E0 galaxy on the Hubble Sequence. There is no clear evidence of tidal features, ongoing mergers, or significant disturbances in its morphology.
