The galaxy presents as an elongated, disk-like structure. It is relatively compact. The galaxy exhibits a bright central region that appears somewhat amorphous. There is a lack of a clearly defined spiral arm structure and the overall morphology seems to be peculiar. There is some indication of faint, extended emission or tidal features. The galaxy has an overall irregular morphology, with potential disturbances in its structure. This suggests possible recent interactions or mergers. There is some color variation within the galaxy, with the central region being bluer, and the outer regions trending more towards redder hues. This could be indicative of varying stellar populations or dust content across the galaxy.
