The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a radial gradient in luminosity, decreasing from the core outwards. The color appears predominantly yellow-red, suggesting an older stellar population and a relatively low rate of current star formation. There is a slight elongation in the galaxy's shape, with a minor suggestion of a disk, but the overall structure is dominated by its spheroid. There is no visible evidence of recent or ongoing major merger activity or significant tidal disturbances. The galaxy appears to be relatively isolated within its immediate surroundings, without any prominent companion galaxies or interacting features.
