The galaxy presents as an irregular form. The primary body exhibits a bright, centrally concentrated core, surrounded by a more diffuse halo of light. This halo appears to be relatively smooth in texture. A smaller, distinct luminous region is visible towards the periphery, which may indicate a tidal interaction or potential merging event. Overall, the galaxy does not display a clear spiral or elliptical structure, suggesting a complex morphology. There is an apparent asymmetry in the distribution of light, further indicating a possible ongoing interaction or recent disturbance. The colour of the galaxy is consistent. The intensity of the light suggests that a significant amount of star formation may be occurring within. The absence of clearly defined spiral arms or a prominent galactic disk reinforces its classification as an irregular galaxy.
