The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decline in brightness towards the outer regions, lacking any obvious spiral arm structures or distinct features. There is an indication of slight elongation of the galaxy along a preferential axis. The color profile suggests a population of older stars, as evidenced by the redder hue, concentrated towards the center. There is little sign of active star formation across the main body of the galaxy.
