The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The overall shape is generally round. There is a noticeable radial gradient in luminosity, with the central region exhibiting the highest surface brightness, indicative of a dense stellar population. The color profile suggests the presence of older stars and a lack of significant recent star formation. Some slight blue hue is visible on the outskirts of the galaxy. There is no apparent evidence of a distinct disk structure or spiral arms. There is no sign of major mergers or disturbances of the galaxy structure.
