The galaxy presents a largely smooth morphology. It has a dominant central bulge, appearing somewhat spheroidal with an intermediate ellipticity. The light is concentrated in the central region, gradually fading outward. The color profile suggests a relatively old stellar population, exhibiting a redder hue in the core region and a slightly bluer component further out, which could be indicative of a more recent, though likely limited, star formation episode in the disk. No spiral arm structures are clearly discernible. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. There may be some minor disturbances, but the galaxy appears relatively settled.
