The galaxy presents as a relatively compact object with a bright central bulge or core. The primary coloration of the galaxy is a blue-green hue, indicative of recent star formation activity and the presence of ionized gases. The central region is intensely luminous, suggesting a high concentration of stars and possibly an active galactic nucleus.

Extending horizontally from either side of the central core are two distinct, fainter features or arms. These extensions appear more reddish or yellowish in color compared to the central region. This color difference may indicate the presence of older stellar populations, dust lanes, or regions of less active star formation.

There is evidence of structural disturbance in the disk or outer regions of the galaxy. The morphology is not entirely smooth and symmetrical, hinting at possible tidal interactions, a recent merger event, or internal dynamics that have disrupted the galaxy's overall structure. The general shape seems to be elliptical.