The galaxy presents a slightly elongated, cigar-shaped morphology. It exhibits a smooth appearance with a concentrated central region, likely a bulge, that emits a brighter, bluer light. The galaxy appears to be relatively undisturbed, with no obvious signs of a major ongoing merger or significant tidal distortions. Fainter light extends from the main body, suggesting the presence of a diffuse halo. There might be a slight asymmetry in the outer regions, possibly hinting at a minor interaction or internal dynamics. The overall color profile indicates a population of older stars, as well as some regions of ongoing or recent star formation.
