The galaxy presents a primarily smooth morphology, appearing largely elliptical in shape, though there is a subtle suggestion of a disk component. The central region exhibits a high degree of concentration, with light intensity decreasing gradually toward the outer edges. There's a faint, broad halo surrounding the main body of the galaxy. The overall color profile suggests intermediate star formation activity, as indicated by a balance of blue and red hues within the galaxy's structure. There are no apparent signs of significant tidal disturbances or ongoing major mergers; any potential interactions appear minor and do not substantially disrupt the galaxy's overall form. The galaxy appears relatively isolated in its immediate vicinity.
