The galaxy appears as a centrally concentrated, relatively smooth object with a generally round morphology. The central region exhibits a yellowish-white hue, suggesting a population of older stars. There is a faint, less concentrated disk component surrounding the central bulge, exhibiting subtle color variations. No distinct spiral arm structures are discernible; the galaxy displays a largely featureless and homogenous appearance. There are no signs of a major ongoing merger event or significant tidal disturbances, although some minor asymmetry may be present. The galaxy has a substantial size and a correspondingly large estimated mass. The colors suggest a relatively low star formation rate, and the light is dominated by older stellar populations.
