The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The galaxy exhibits a generally round shape, with only a very slight elongation along one axis. The core region is bright and yellowish-white, with the intensity of light decreasing gradually outwards to its faint edges. No distinct spiral arms or prominent dust lanes are visible, suggesting a lack of significant ongoing star formation. There is no evident sign of any mergers or tidal disturbances. The morphology suggests a galaxy that is likely to be in a relatively late stage of its evolution. The lack of blue color indicates the stellar population is likely dominated by older, redder stars.
