This galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile with no apparent spiral arm structure or prominent dust lanes. The core region displays a concentrated, bright intensity, suggesting a high stellar density. The galaxy's color appears relatively uniform across its extent, with a slight red-yellow hue, indicative of an older stellar population. There is a faint, irregular structure located in close proximity to the central galaxy, which might be a sign of a minor gravitational interaction, though it could also be a background object. Overall, this galaxy appears to be a mature system, undergoing a potentially weak merging interaction.
