The galaxy presents as an elliptical morphology, displaying a smooth, featureless structure. Its overall shape is elongated, exhibiting a cigar-like appearance. The light distribution is centrally concentrated with a gradual decrease in luminosity towards the outer edges. A subtle color gradient is observed, transitioning from a slightly yellowish hue in the central region to a bluer color in the outer regions, suggesting a potential variation in stellar population or age. There is no visible evidence of spiral arms, dust lanes, or ongoing merging activity. The galaxy appears to be relatively isolated and undisturbed.
