The galaxy presents a generally smooth, elliptical morphology. It appears nearly circular. The galaxy exhibits a concentrated central bulge that dominates the light profile. There is little evidence of significant spiral arm structure or dust lanes. Its color suggests an older stellar population, with fewer signs of ongoing active star formation, although light in other bands indicates some star formation. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interactions or recent mergers. The object presents an even light profile that is highly concentrated in its center, implying a high Sersic index.