The galaxy presents as a primarily smooth, elliptical structure. Its color profile indicates an older stellar population with a dominant reddish-yellow hue, suggesting reduced recent star formation activity. A faint, subtle disk-like structure is potentially visible with possible merging features, perhaps indicating some minor gravitational interaction or recent accretion event. There is some indication of tidal tails or other disturbances. The galaxy exhibits moderate luminosity. Overall, it appears to be a relatively evolved system, potentially nearing the end of its star-forming phase.
