The galaxy presents as a moderately bright, resolved object. It exhibits a generally elliptical morphology, though not perfectly circular, showing some deviation toward an elongated shape. The light distribution appears relatively smooth, with no prominent spiral arm structures or significant dust lanes visible. The color index suggests the presence of a population of older stars, as indicated by its overall reddish hue, with g-band magnitude brighter than r-band magnitude, and r-band magnitude brighter than z-band magnitude.. There's no immediately apparent evidence of a major ongoing merger, although a subtle asymmetry might suggest a minor interaction or tidal disturbance in the past, with no merging currently, but a likely minor disturbance. The size of the galaxy appears relatively small, indicating either a dwarf galaxy or a larger galaxy at a significant distance.
