The galaxy presents as a centrally concentrated, largely spheroidal object. The core exhibits a bright, yellowish hue, suggesting a significant population of older stars. The overall structure appears smooth, with no immediately obvious spiral arm features. There is some faint extension of light around the central bulge, hinting at a diffuse halo component. The galaxy's red color indicates that a considerable amount of its light may be emitted at the redder part of the spectrum, possibly due to redshift. A smaller object is visible to the left of the main galaxy.
