This galaxy appears as a compact, relatively bright object with a smooth light distribution. There is evidence of a disk structure. The galaxy exhibits a distinct color gradient, with a bluish central region suggestive of ongoing star formation activity. A faint, reddish ring surrounds the blue core, which may indicate a population of older stars or dust extinction. Based on the overall morphology, the galaxy does not appear to be undergoing any major merging events or significant tidal disturbances.
