This galaxy exhibits a morphology dominated by a smooth, elliptical-like structure. There's a slightly elongated shape to the galaxy; it is somewhat cigar-shaped. The galaxy presents a dominant central bulge with a concentrated, bright core suggesting a high stellar density. The light distribution appears relatively uniform across the galaxy, with no strong evidence of spiral arm structures or prominent dust lanes. There are some indications of minor disturbances or potential interactions, but no obvious signs of a major merger or tidal tails. The overall color is consistent with an older stellar population; the light has a yellow-red hue, which generally indicates the presence of older, redder stars rather than young, blue stars associated with active star formation.
