The galaxy presents as a largely featureless, elliptical object. It exhibits a high degree of central concentration with a smooth, diffuse profile extending outwards from a bright, moderately compact core. The light distribution suggests a relatively homogenous stellar population, with a notable absence of distinct spiral arms or prominent dust lanes. The overall shape appears nearly circular, indicative of a spheroidal system viewed close to face-on. There is a subtle color gradient, with the core appearing slightly yellower than the outer regions, potentially indicating a higher concentration of older, redder stars in the central bulge. The lack of obvious morphological disturbances suggests it is a relatively undisturbed system, not currently undergoing major merger activity. Based on the color and morphology, this galaxy is likely an evolved system with a relatively low rate of ongoing star formation.
