The galaxy exhibits a flattened, elliptical morphology, with a major axis significantly longer than its minor axis. The central region presents a concentrated luminosity, appearing smooth and relatively featureless. The disk shows a distinct tilt relative to our line of sight. The observed color gradient transitions from a bluer hue towards the outer edges, suggestive of recent or ongoing star formation, to redder tones in the central bulge, indicative of an older stellar population. The integrated light profile appears well-fit by a Sersic profile. There may be a very minor tidal disturbance. Overall, this galaxy likely hosts a moderate stellar mass and star formation rate. The galaxy is likely a spiral galaxy, but its disk-like structure may be obscured by dust and/or inclination.
