The galaxy presents a largely smooth and rounded morphology. It is predominantly elliptical in shape, showing a gentle gradient of light intensity from a bright, concentrated central bulge outwards to a fainter halo. There is minimal discernible structure within the disk, and there are no prominent spiral arms or bar features visible. The galaxy appears to be a relatively undisturbed system, showing no signs of ongoing major merger activity or significant tidal distortions. There may be a subtle hint of internal disc structure or a minor interaction, but these are not strongly defined. The colors are composed of light to moderate blues and reds, indicating a varied stellar population, likely dominated by older stars but with the possibility of some ongoing star formation.
