The galaxy presents as a relatively smooth elliptical morphology, with a high degree of central concentration. A bright nucleus is visible, surrounded by a diffuse halo of light extending outwards. There is a slight elongation, suggesting a deviation from a perfectly circular shape, appearing somewhat in between round and cigar-shaped. No distinct spiral arms or significant dust lanes are immediately apparent. There is a suggestion of faint, diffuse features in the outer regions, but these are subtle. The overall color appears to be on the redder end of the spectrum. There is no strong indication of ongoing major merger activity or significant disturbances in its structure, though some minor disturbances are not fully ruled out.
