The galaxy presents as a centrally concentrated, smooth object. It exhibits a nearly circular morphology, with a slight elongation discernible. The light profile appears centrally peaked, suggesting a substantial bulge component. Color gradients are subtle, with a slightly bluer hue extending from the core outwards, which could indicate some ongoing, albeit subdued, star formation activity in the outer regions. No distinct spiral arms or other prominent features such as bars or rings are visible. There's no strong evidence of any recent major merger events based on tidal tails or other significant morphological disturbances. The overall impression is that of a relatively massive and evolved galaxy.
