The galaxy presents as a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that dominates its overall luminosity. The color profile suggests an older stellar population, leaning towards redder hues in the core with a gradient towards slightly bluer shades in the outer regions.  There is no clear spiral structure or bar visible. The galaxy appears to be relatively isolated with only slight indications of tidal disturbances, if any at all. It appears to be relatively undisturbed, maintaining a mostly regular structure. The object is elongated, but could be described more as in between a round and cigar shape. There is a high probability that this galaxy is not merging with another galaxy, or experiencing any other kind of major disturbance.