The galaxy presents as a single, relatively smooth object. It appears somewhat spheroidal in shape, exhibiting a high degree of roundness. There is no obvious central bulge nor spiral arm structure visible in this observation, although the resolution is limited. There might be a slight variation in brightness across the galaxy's surface, but overall, it is relatively uniform. There is no evidence of a significant ongoing merger or major tidal disruption. Based on the observed color profile, this galaxy seems to be composed of a population of older stars. This is also evident based on the relatively low star formation rate. There is no significant dust lane or other obscuring feature visible.
