The galaxy presents as a moderately luminous, early-type system, possibly an elliptical galaxy or a lenticular galaxy seen at a slight inclination. The core exhibits a concentrated luminosity profile, appearing smooth and without any obvious spiral arm structure. The galaxy displays a subtle elongation, deviating slightly from a perfectly circular shape. The color index suggests a population of older stars, evidenced by the redder hue. There is no obvious dust lane or significant star formation activity visible in the image. The overall morphology appears relatively undisturbed, with no apparent signs of ongoing major mergers or significant tidal interactions. Subtle color gradients are present within the galaxy, with the central region exhibiting a slightly yellower tint compared to the outer regions. There are possible minor disturbances or asymmetries at the outer edges of the galaxy, but these appear minimal.
