The galaxy presents as a moderately sized, elliptical object with a relatively smooth light distribution. The central region exhibits a high surface brightness, appearing as a concentrated bulge. The luminosity appears brightest in the redder bands with a slight shift toward green. The overall color is indicative of a mature stellar population, possibly dominated by older, redder stars. There is some asymmetry visible in the outer regions, with one faint filament, suggesting a possible interaction with other galaxies or possibly a minor disturbance due to a past merger event. There is no obvious strong spiral structure visible, but there are hints of a disc.
