The galaxy presents a generally smooth, centrally concentrated morphology. The light profile is relatively featureless with a dominance of a bright central bulge, exhibiting a fairly elliptical shape, although with a moderate degree of roundness. There is little evidence of significant disk structure or spiral arms. The galaxy appears to be relatively undisturbed, showing no strong signs of tidal interactions or ongoing mergers. There is potentially some minor disturbance in the surrounding regions. It exhibits colors consistent with a redder stellar population and relatively low levels of ongoing star formation.
