The galaxy presents as a somewhat elliptical, moderately luminous object. It exhibits a smooth light distribution, with a concentrated central bulge and a diffuse, extended halo. The color profile suggests an older stellar population, leaning towards redder wavelengths. There are hints of possible minor disturbances in the halo, although no prominent tidal tails or clear signs of a major merger event are readily apparent. The galaxy appears relatively isolated, showing no obvious signs of strong interaction with neighboring galaxies.
