The galaxy presents as a slightly elliptical, centrally concentrated object. Its core region exhibits a high surface brightness with a yellowish-white hue, suggesting an older stellar population. The light distribution gradually decreases outward from the core, transitioning into a fainter, bluer halo. This halo appears relatively smooth, with minimal evidence of distinct spiral arm structures or prominent star-forming regions within its structure. There is a very slight asymmetry, suggesting that the galaxy may be interacting with another object or that it has undergone a past merger. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy, possibly an elliptical or a lenticular galaxy.
