This galaxy exhibits a primarily smooth morphology, indicating a likely elliptical or lenticular classification. The galaxy's shape appears somewhat elongated, leaning more towards an "in-between" or slightly cigar-shaped profile rather than perfectly round. A brighter central bulge is apparent, surrounded by a more diffuse halo. There is a faint hint of a possible disk structure within the halo, with some subtle color variations present. The galaxy appears to be relatively isolated, showing no strong evidence of ongoing major mergers, though a minor disturbance on one edge might indicate a past interaction or accretion event. Based on its general color profile and morphology, it appears to be a relatively massive galaxy with a modest rate of star formation, leaning towards a redder color, which typically correlates to older stellar populations.
