The galaxy presents as a relatively smooth, lenticular object, though not perfectly elliptical. Its overall color profile suggests a relatively mature stellar population, exhibiting a redder hue with some subtle color gradients within the galactic structure. There is a suggestion of a slight bulge, where the central region appears somewhat more concentrated. There are some minor hints of possible tidal disturbances or faint, extended features suggesting recent or ongoing interactions, though the bulk of the galaxy is smooth. Its moderate size and luminosity suggest an intermediate-mass system with signs of on-going star formation.
