The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated morphology. The core region displays high luminosity, suggestive of a significant concentration of stellar mass and/or an active galactic nucleus. The radial surface brightness profile appears to decrease smoothly from the center outwards. The galaxy is moderately elongated, with an aspect ratio indicating a shape that is in between circular and cigar-shaped. The lack of well-defined spiral arms or prominent dust lanes supports the classification of this galaxy as an early-type system. There might be some minor disturbances visible. The color gradient suggests a population of older stars. Overall, the galaxy appears to be relatively undisturbed with no major signs of interaction.
