The galaxy presents as a smooth, elongated elliptical shape. Its core region exhibits a concentrated, bright luminosity. The galaxy appears largely featureless, with no readily discernible spiral arms or distinct dust lanes. The light distribution suggests a relatively uniform stellar population. The overall color is consistent with an older stellar population, lacking prominent blue hues indicative of active star formation. There is a subtle gradient in surface brightness from the center outwards. The major axis is significantly longer than the minor axis, suggesting a considerable ellipticity. There is no visual evidence of ongoing merging activity or significant tidal disturbances.