This galaxy presents as a relatively small, elliptical structure with a bright central bulge. The galaxy is observed at a high inclination, appearing as a flattened disk. It exhibits a smooth light distribution, with a concentrated nucleus. The galaxy appears largely undisturbed, without obvious signs of major merging activity or tidal features. There may be some low level disturbances present. The galaxy's color profile suggests a blue hue, which could indicate the presence of younger stars. This observation does not fully align with the observed smoothness and ellipticity, which might signify a more evolved stellar population.
