The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape is elliptical to slightly lenticular, displaying a moderate degree of ellipticity. There is no apparent spiral structure or distinct disk component visible in the image. The core exhibits a bright, concentrated luminosity that fades gradually towards the outer regions. Color gradients are subtle, with a suggestion of a redder hue in the central bulge and a marginally bluer tinge in the outskirts. There are no obvious signs of recent or ongoing major mergers or significant tidal disturbances, although subtle irregularities could indicate minor interactions or internal activity. The galaxy appears relatively isolated.