The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated core region that gradually diffuses outward. There is an apparent lack of distinct spiral arm structures. The color profile suggests a population of older stars, evidenced by the reddish-yellow hue, which could indicate relatively low levels of on-going star formation. A slight asymmetry or disturbance is noted in the outer halo, potentially indicative of a past minor merger event or tidal interaction. The galaxy appears moderately round, but with a slight deviation from perfect sphericity. There is some indication of a fainter, diffuse structure possibly associated with the galaxy, though the image resolution limits detailed analysis.
