The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing elongated but not dramatically so. The color profile suggests a dominant population of older stars, evidenced by the yellow-orange hue concentrated towards the center. There is a slight color gradient, with a subtle shift toward bluer tones in the outer regions. There is no apparent spiral arm structure or significant dust lane obscuration. There may be some subtle disturbances suggesting possible past merger events or tidal interactions, but they are minor. 
