The galaxy exhibits a bright, centrally concentrated core, suggesting the presence of a significant stellar population. The color profile indicates a bluer hue in the central region, potentially indicative of younger stars or ongoing star formation. A faint, extended disk-like structure is visible, although it appears somewhat disturbed or irregular. There is evidence of possible tidal features or minor disturbances within the extended structure, perhaps indicating a recent or ongoing interaction with another galaxy. The overall morphology leans towards a disturbed spiral or an irregular galaxy due to the lack of clearly defined spiral arms and the noted disturbances.
