The galaxy presents as an elongated, elliptical structure. It exhibits a relatively smooth light distribution, with a concentration of luminosity toward the center, forming a bright core. The color profile suggests an older stellar population, leaning towards redder hues in the central regions. The galaxy appears to be relatively isolated, with no obvious signs of recent major mergers or tidal interactions, although some minor asymmetry in the outer regions cannot be ruled out. The overall morphology suggests a system dominated by random stellar motions.