The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, concentrated light profile. The core region appears quite bright and shows a yellowish-white hue, indicative of an older stellar population dominating the center. Moving outwards from the core, the light gradually diminishes, transitioning to a slightly more reddish tint. There is little evidence of distinct spiral arms or prominent dust lanes within the visible structure. The overall shape is somewhat elongated, although not dramatically so, displaying an intermediate ellipticity. There may be a faint, diffuse halo surrounding the main body, extending subtly beyond the more concentrated regions of the galaxy, which is consistent with moderate star formation.
