The galaxy presents as a single, concentrated luminous body. Its overall shape is generally round and smooth, with a radial gradient in luminosity. The core region exhibits a higher surface brightness, suggesting a concentrated stellar population or active galactic nucleus. The galaxy is slightly elliptical and is not edge-on. There is faint, diffuse emission extending outward from the central region; with hints of faint arms. There is no strong evidence of ongoing major mergers, although slight distortions may be present in the outer halo. The color profile suggests a somewhat older stellar population, with a yellowish hue. The image does not show any distinct dust lanes or prominent HII regions.
