The galaxy presents as a single, concentrated light source with a generally elliptical morphology. A smooth, centrally concentrated bulge is visible, exhibiting a yellow-orange hue suggesting an older stellar population. A faint, diffuse halo surrounds the central bulge, extending outwards with a gradual decrease in surface brightness. The lack of clearly defined spiral arms or distinct features suggests this is likely an early-type galaxy. The light appears relatively uniform, indicative of a well-mixed stellar population. There is no obvious sign of ongoing major star formation, which supports a classification as an elliptical galaxy. The object appears undisturbed, showing no clear evidence of any recent or ongoing mergers or tidal interactions.
