The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge region dominates the light profile, exhibiting a yellowish-orange hue suggestive of an older stellar population. The outer regions display a faint disk-like structure. A slightly more pronounced red color, suggestive of potentially older or dust-obscured regions, are situated off center to either side of the galaxy. There is a suggestion of minor disturbances, such as a subtle tidal feature, on one side of the galaxy. However, no significant ongoing merger event or major disruption is apparent. The galaxy appears relatively isolated, with no clear evidence of strong gravitational interaction with nearby companions in this field of view.
