The galaxy appears as a somewhat elongated, diffuse object with a smooth texture. There is little evidence of spiral arm structure or significant dust lanes. The galaxy presents a centrally concentrated luminosity profile, suggesting a bulge component is present. The color is a relatively uniform pale blue-white across the galaxy, possibly indicative of a population of older stars, but with hints of recent star formation. There is no obvious tidal debris or other signs of recent major merger activity, although a slight asymmetry could indicate a minor interaction in the recent past. The overall impression is of a galaxy undergoing relatively quiescent evolution. Based on the faintness, it is expected to be relatively distant.
