The galaxy presents a relatively compact morphology, appearing somewhat amorphous with a bright central concentration. There is a noticeable blue hue emanating from the central region, which may indicate the presence of younger stellar populations or ongoing star formation. The outer regions of the galaxy appear less defined and fainter, with subtle extensions that suggest possible tidal features or disturbances. Overall, the galaxy doesn't exhibit a clearly defined disk structure, and it could be an irregular galaxy, or potentially an early-type galaxy with some unusual features. There may be some signs of possible minor interactions or disturbances affecting the galaxy's overall structure.
