The galaxy presents as a structured system with a prominent central bulge, potentially indicative of an older stellar population. Surrounding this bulge is what appears to be a disk component, although the image resolution limits detailed morphological classification. Color variations within the disk suggest the presence of regions with varying stellar populations or dust content. There is evidence of some disruption within the structure, which may be the sign of a minor ongoing merger with a smaller, compact object in close proximity to the disk on its right. The galaxy exhibits a relatively smooth profile, with an apparent axis ratio suggesting it is viewed at an angle from face-on, though not edge-on. The limited resolution obscures any detailed spiral arm structure or other fine-scale features, and the possibility of this being a lenticular galaxy cannot be ruled out. The estimated size of the galaxy is relatively small. Overall, the galaxy appears to be an intermediate-mass system with ongoing or recent interaction and moderate star formation.
