The galaxy presents as a somewhat elongated, lenticular-shaped object with a smooth, diffuse appearance. The central region exhibits a high surface brightness and a yellowish-white hue, indicative of an older stellar population. The outer regions display a fainter, bluish tint suggesting the possibility of some younger stars, although star formation activity seems minimal based on the general smoothness and lack of distinct spiral arms. The galaxy is slightly cigar shaped. There is no discernible evidence of significant disturbances due to mergers or tidal interactions. Overall, this appears to be a relatively quiescent galaxy, transitioning from a spiral to elliptical form, based on its structure.
