The galaxy presents as an elliptical system with a smooth, centrally concentrated light profile. The core exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outward, the galaxy appears to fade gradually, with a more diffuse, indistinct halo. The overall shape is elongated, displaying a cigar-like morphology, without any prominent spiral arms or disk features. There are no apparent signs of major mergers or significant tidal disturbances. The galaxy's red color indicates that star formation is likely suppressed or has ceased altogether.
