The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, diffuse light distribution across its main body. The core region is noticeably brighter and appears yellowish, suggesting an older stellar population dominates this area. Moving outwards from the core, there's a subtle transition to a bluer hue in the galaxy's outskirts, hinting at the presence of younger, hotter stars, although these do not appear to be in well-defined spiral arms. The galaxy displays evidence of a possible minor disturbance. The overall shape is somewhat rounded but not perfectly spherical, with a slight elongation. There is a faint suggestion of an interaction or minor merger event occurring, with some disturbed light distribution on one side of the galaxy. The galaxy is relatively compact. There are no strong indicators of active star formation, such as prominent HII regions or dust lanes, implying a relatively quiescent state.
