The galaxy presents as an elliptical or lenticular type, with a smooth, generally featureless appearance. The light profile suggests a centrally concentrated bulge, decreasing in intensity with radial distance. There is a slight elongation, indicated by a non-perfectly round shape. The galaxy's color index suggests a population of older stars, with a redder hue concentrated towards the center. There are no apparent spiral arms or significant dust lanes visible. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. Faint hints of possible minor disturbances are visible at the outer edges, but the galaxy generally appears stable and relaxed in its structure. Its estimated size is on the order of several kiloparsecs. Based on color and lack of prominent star-forming regions, the star formation rate appears to be low.
