The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing somewhat elongated but generally rounded. There's a noticeable bulge component at the center, exhibiting a high surface brightness. The light distribution gradually decreases outwards from the core, fading into a more diffuse halo. There appears to be little evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a yellowish-white hue, suggestive of an older stellar population. Faint, diffuse light extends beyond the main body, indicating a possible stellar halo. There are no obvious signs of a major ongoing merger or tidal disturbance, although subtle asymmetries in the outer regions cannot be entirely ruled out.
