The galaxy presents as a moderately luminous elliptical or lenticular type, exhibiting a generally smooth and symmetrical morphology. There is a concentrated central bulge. The light profile appears to diminish gradually from the core, and there is no evidence of spiral arms, bar structure, or significant dust lanes. A slight reddish hue dominates the central region, potentially indicating an older stellar population with reduced recent star formation. The outer regions display a more greenish tint suggesting a younger stellar population on the outskirts. There are no signs of tidal disturbances or ongoing major mergers. The galaxy appears fairly isolated with no immediate interacting companions visible in this field of view. The object's overall structure suggests it is a relatively evolved system.
