The galaxy presents as a generally smooth, elliptical-like morphology, exhibiting a concentrated central bulge that transitions smoothly outward. The color profile suggests an older stellar population, with a dominant yellowish-orange hue at its core, fading into slightly bluer tones in the outer regions, though the blue contribution remains minimal. There is little indication of spiral arm structures or significant dust lanes. The overall symmetry is high, and there is no visible evidence of any ongoing major mergers or tidal disturbances. The galaxy appears to be relatively isolated, with a high probability that it is not merging. The general roundness suggests a low inclination angle relative to our line of sight. It is a medium sized galaxy.
