This galaxy appears as a single, relatively smooth object. It exhibits a generally elliptical shape, with a high degree of roundness. The galaxy's light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. There is no discernible spiral arm structure or evidence of a prominent disk component. Faint, extended features might be present, indicating possible tidal interactions or recent mergers, but they are not distinct. There is no clear indication of ongoing star formation within the visible spectrum; the light is dominated by older stellar populations. The galaxy exhibits a consistent, single color with little variation across its surface. There appears to be no significant dust lane obscuration.
