The galaxy presents a generally smooth and elliptical morphology. The color gradient transitions from a yellowish core to a redder outer region, indicating a stellar population that is likely older and more evolved in the central region. No distinct spiral arm structures or prominent dust lanes are visible. A slight asymmetry is apparent in its shape, suggesting a possible past interaction or minor disturbance. The galaxy exhibits a relatively concentrated light profile, with a significant fraction of its total luminosity emanating from a compact central area. Its size appears relatively moderate. Overall, this galaxy appears to be a relatively massive and passive elliptical galaxy at a considerable distance.
