The galaxy presents a smooth, elongated morphology, consistent with an elliptical or lenticular type. Its color profile suggests an older stellar population, with a dominant yellow-orange hue concentrated towards the galactic center. There is no prominent dust lane or spiral arm structure visible. The galaxy appears undisturbed, lacking any obvious signs of tidal interactions or recent merger events. The overall smooth profile indicates a system dominated by older stars and a relatively quiescent star formation rate. The shape of the galaxy is noticeably elongated along one axis, resembling a cigar shape. This is a relatively large and massive galaxy.
