This galaxy exhibits a relatively compact morphology. It appears to have a bright, concentrated core, possibly indicating the presence of an active galactic nucleus or a dense stellar population within the central region. The galaxy's overall structure is somewhat irregular, hinting at potential past or ongoing interactions or mergers. Faint extensions or tidal features are suggested surrounding the main body. A subtle disk-like structure may be present. The color distribution reveals a mixed stellar population, with a relatively redder component towards the outer regions and bluer hues concentrated in the core, possibly indicating on-going star formation in that region. There seems to be some disturbance or asymmetry in the outer disk, which could be caused by interactions with another galaxy.
