The galaxy presents a primarily smooth morphology, exhibiting a centrally concentrated luminosity profile that diminishes gradually towards its outer regions. Its overall shape appears largely spheroidal, with a high degree of roundness. No strong indications of spiral arms or a significant disk component are readily apparent in the available imagery. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although subtle irregularities cannot be ruled out with this image resolution. The galaxy's color suggests an evolved stellar population, lacking the blue hues associated with vigorous recent star formation. Overall, the galaxy appears to be a relatively undisturbed, evolved system, likely an elliptical or lenticular galaxy.
