This galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge, brightest in the yellow-orange wavelengths, suggesting a population of older stars. Fainter, diffuse light extends outwards from the core. While the galaxy presents primarily a spheroidal shape, there is a slight elongation or cigar-like quality noticeable in its overall form. There are no readily apparent signs of strong tidal disturbances or major merger events impacting the overall structure, although some minor asymmetries within the extended halo cannot be ruled out.
