The galaxy presents as a largely featureless, elliptical form. It displays a smooth, concentrated light profile, indicative of an older stellar population. Its morphology appears generally undisturbed, with no prominent signs of tidal interactions or ongoing major mergers. The galaxy exhibits a slight elongation along one axis, deviating minimally from a perfect circular shape. Overall color suggests a redder spectral energy distribution, consistent with a population of evolved stars and a relatively low rate of star formation. Faint, diffuse light extends outwards from the central region, gradually fading into the background. There is a hint of minor asymmetry, but further, higher-resolution imaging would be required to determine its nature.
