The galaxy presents a predominantly smooth morphology, appearing largely featureless upon visual inspection. It exhibits a generally elliptical shape, tending toward roundness. The light is concentrated towards the center of the galaxy, indicating a prominent bulge. The color profile suggests an older stellar population, with a shift toward redder hues in the central bulge. Overall, the galaxy appears relatively isolated, showing no obvious signs of major interaction or ongoing merger activity, although some minor disturbances cannot be ruled out given the resolution. There is an apparent asymmetry, with a faint, possibly tidal feature or minor distortion, extending from one edge of the galaxy, requiring deeper investigation.
