The galaxy presents as a relatively compact structure with a smooth, diffuse light distribution. It exhibits a generally elliptical morphology with a moderate degree of roundness. The core appears bright and concentrated, with a color profile suggesting an older stellar population, potentially dominated by redder giant stars. There is little evidence of distinct spiral arm structures or prominent dust lanes. There may be some subtle irregularities or minor disturbances in the outer regions, but the overall structure appears largely undisturbed, lacking indications of ongoing major mergers. Based on the estimated size, this is a substantial galaxy. Given the color and relatively smooth light distribution, the galaxy may be in a relatively passive stage of star formation.
