The galaxy presents as a roughly elliptical structure with a smooth, diffuse light distribution. The core region appears slightly brighter, suggesting a concentration of stars towards the center. No distinct spiral arms or prominent dust lanes are visible. The galaxy exhibits a somewhat elongated shape. The color profile appears relatively uniform, with a slight yellowish tint. There is no obvious evidence of active galactic nuclei activity or recent major mergers, such as tidal tails or strong asymmetries in the light distribution. The galaxy appears relatively isolated, with no other large galaxies in close proximity suggesting possible interactions. However, there are a number of smaller neighboring galaxies. Overall, the galaxy is consistent with being an early-type galaxy, specifically, an elliptical.
