The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its overall shape approximates a circular form. The light distribution is dominated by yellowish hues emanating from the core, possibly indicating an older stellar population. There is little evidence of spiral arms or significant dust lanes. A slight color gradient is observed, shifting from a yellow center to a more reddish periphery. No major disturbances or signs of ongoing mergers are readily apparent in its structure, and its stellar formation activity appears subdued.
