This galaxy appears to be a relatively compact object, exhibiting a somewhat elliptical morphology. The core is bright and concentrated, possibly indicating a significant central mass concentration. Surrounding the core, there's evidence of a disk-like structure. The disk appears to be slightly disturbed or asymmetric, with faint extensions or tidal features visible, suggesting past or ongoing gravitational interactions. The galaxy displays a range of colors; the central region is bluer, potentially indicating active star formation, while the outer regions appear redder, which could suggest an older stellar population or dust extinction. Overall, the galaxy exhibits characteristics of a system that may be undergoing a minor merger or experiencing some form of external disturbance.
