The observed galaxy presents a relatively compact morphology with a moderate angular size. The central region displays a high degree of smoothness and a bright, concentrated core, suggestive of an elliptical or lenticular classification. There is a faint, diffuse extension surrounding the core, possibly indicating a stellar halo or tidal features. Visual inspection suggests some level of disturbance within the galaxy, indicating the possibility of a minor merger or tidal interaction. The color gradients from the core to the outer regions suggest variations in stellar populations or dust content. Overall, the galaxy exhibits characteristics of an early-type system that may be undergoing some level of interaction.
