The galaxy presents as a roughly elliptical structure, elongated along its major axis. Its color profile indicates a bluish hue, suggesting a population of relatively young, hot stars and active star formation. The light is concentrated towards the center, which fades into a diffuse halo without distinct spiral arm features. The overall morphology is largely undisturbed, showing no evidence of recent major mergers or strong tidal interactions, though some minor asymmetry might be present on one edge. This is indicative of a relatively settled galactic disk galaxy.