The galaxy presents as a relatively smooth, rounded structure. Its color appears predominantly blue-white, with a central concentration that suggests the presence of a substantial stellar population. There is little evidence of spiral arms or significant disk features, indicating a more elliptical or lenticular morphology. The uniform appearance and lack of distinct substructures suggest limited on-going star formation and potentially an older stellar population. There are no signs of any ongoing major mergers or significant tidal disturbances.