The galaxy presents a reddish-orange hue overall, suggestive of an older stellar population. The morphology appears primarily elliptical, lacking a prominent disk structure. There is a possible, but uncertain, minor disturbance or subtle irregularity in the light distribution, indicating a potential past or ongoing interaction event. The central region is brighter than the outer regions with a relatively smooth appearance; some light appears more concentrated in the center. There is potentially some tidal activity or disturbances.
