The galaxy presents as a primarily smooth object, with a significant fraction of its light concentrated in a central bulge. The shape approximates an ellipse, appearing somewhat cigar-shaped with an intermediate axis ratio. There is a subtle color gradient, with the central region exhibiting a yellowish-orange hue, possibly indicating an older stellar population. The outer regions appear slightly bluer, suggesting the presence of some younger stars. There is no apparent evidence of a strong disk or spiral structure, nor of any major mergers or tidal disturbances, although some minor irregularities in the outer halo cannot be entirely ruled out at this resolution. The galaxy seems to have a high estimated mass, with a low to moderate star formation rate.
