The galaxy presents as a centrally concentrated object with a relatively smooth, unresolved morphology. Its color profile suggests a dominant population of older stars, with a reddish-yellow hue concentrated towards the core and a slight shift towards bluer tones in the outer regions. The galaxy appears elliptical in shape, though with only a slight deviation from perfect circularity. There is no clear evidence of spiral arms, a bar, or any major morphological disturbances indicative of recent merger activity. The observed light distribution is consistent with a quiescent galaxy that has largely ceased forming new stars.