The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated light profile. The core region shows a bright, yellowish-white hue, suggesting an older stellar population. There is a noticeable falloff in intensity outwards from the core. The galaxy's shape appears roughly circular, though a slight elongation is not entirely excluded. Faint, diffuse extensions of light are present around the central region, possibly indicating a halo of older stars or a disrupted structure from a minor merger event. The galaxy does not show any obvious spiral arm structures, dust lanes, or significant signs of recent star formation. Subtle variations in color within the outer regions are present, however the overall impression is of a uniformly old, relaxed stellar population. There are some possible signs of minor disturbance to the central galaxy.
