This galaxy presents as a relatively smooth object with a high degree of central concentration. It appears nearly circular in projection, displaying minimal flattening or ellipticity. The galaxy exhibits a prominent bulge component, suggested by a bright, concentrated core. Fainter, extended structures are visible surrounding the central bulge, hinting at a possible disk or halo. The light distribution suggests a lack of spiral arm structure. There is some color variation, with a suggestion of redder hues in the outer regions and bluer hues more centrally. There might be a minor interaction or gravitational disturbance as suggested by a warp in the light distribution.
