The galaxy presents a predominantly smooth morphology with a concentrated central bulge. The light profile appears diffuse, indicating a lack of distinct spiral arms or a bar structure. The overall shape is generally elliptical, though verging on round, with a suggestion of a slightly elongated or flattened form. There are no signs of major mergers or significant tidal disturbances in the immediate vicinity. The color gradient transitions from a yellowish-white core to bluer hues in the outer regions, consistent with a central population of older stars and potential younger star formation in the periphery. The galaxy appears relatively isolated, with minimal evidence of interactions with neighboring galaxies.
