The galaxy presents as an elongated, cigar-shaped structure, with a smooth, diffuse light distribution. A central bulge is apparent, displaying a more concentrated and warmer hue. The galaxy exhibits an elliptical morphology. No distinct spiral arms or prominent dust lanes are visible. The overall color suggests a relatively evolved stellar population, with a possible presence of ongoing, albeit low, star formation, primarily concentrated within the bulge. There is no clear indication of tidal disturbances or major mergers in the immediate vicinity of the galaxy. The observed characteristics classify it as likely an elliptical galaxy, possibly undergoing a phase of slow evolution.
