The galaxy appears as a relatively compact, elliptical-like structure with a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. A gradual decline in brightness emanates from the center outwards. The outer regions fade to a blue color, implying the presence of some younger, hotter stars, although they contribute only minimally to the overall galactic luminosity. There's no distinct spiral arm structure visible, suggesting either a lack of recent major mergers or the absence of significant gas reservoirs for ongoing star formation. There's no evidence of major morphological disturbances or tidal features, indicating that the galaxy is not currently undergoing a significant merging event.