The object exhibits a generally elliptical morphology with a relatively smooth light distribution. The central region is highly concentrated and bright, appearing nearly spheroidal, suggesting a substantial bulge component. There is some evidence of possible merging activity or tidal disturbances. There is a hint of asymmetry in the galaxy's outer isophotes, which could be indicative of an ongoing minor merger event or interaction with a nearby galaxy. The overall color appears moderately red, implying an older stellar population and reduced levels of recent star formation.
