The galaxy presents as a centrally concentrated, smooth object. Its overall shape is somewhat elliptical, tending toward an intermediate roundedness. The central bulge exhibits a bright, compact core, surrounded by a more diffuse halo of light. Faint extensions are present extending away from the central bulge. There is little evidence of well-defined spiral arm structure or prominent dust lanes. There may be some minor disturbances or tidal features present. The object appears to be experiencing moderate star formation. Color analysis reveals a spectrum that is skewed towards the red end of the spectrum. This may suggest an older stellar population.
