This galaxy appears to be a relatively smooth, elliptical galaxy. The central region exhibits a concentrated, bright core, which graduates into a more diffuse halo. There is a noticeable color gradient, with the core exhibiting a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the center, the color shifts slightly toward the redder end of the spectrum, possibly indicating a population of evolved red giant stars. The overall shape is generally round, with no obvious signs of spiral arms or a distinct disk. There is no clear evidence of recent major merger activity, though there may be very slight irregularities in the outer halo, suggesting possible minor interactions in the past. No significant dust lanes are visible. The light distribution is fairly smooth and even.
