The galaxy presents an elliptical morphology, elongated along a defined axis. The color profile shows a central concentration of light, reddish in hue, suggesting a population of older stars and minimal ongoing star formation in the core. Moving outwards from the center, a subtle shift towards greenish tones is observed, potentially indicating the presence of younger stellar populations or regions of ionized gas, although these features are not sharply defined, but are more indicative of an in-between type. There are no prominent spiral arms or distinct dust lanes visible. The galaxy appears relatively smooth in texture with a somewhat symmetrical structure.
