The galaxy presents as a relatively smooth, elliptical-like structure. It is elongated in shape, appearing cigar-shaped on the sky. The central region exhibits a concentrated luminosity, possibly indicating the presence of an older stellar population. The light gradually diminishes towards the outer regions of the galaxy, suggesting a declining stellar density. There is little evidence of spiral arms or prominent dust lanes, reinforcing its classification as likely elliptical. Overall, the galaxy appears largely undisturbed, exhibiting no signs of major mergers or tidal interactions. There are hints of blue tinges in the outskirts, indicating a small amount of recent star formation, though the star formation activity is generally low. The object has an estimated mass of 10^9.9 solar masses.
