The galaxy presents as a relatively smooth, elliptical or lenticular structure, exhibiting a concentrated central bulge and a diffuse halo. The core region displays a yellowish hue, suggestive of an older stellar population and diminished star formation activity there. Moving outwards from the center, the color subtly shifts towards a slightly bluer tone, indicating the presence of younger, hotter stars in the outer regions, though these regions appear significantly less prominent. No distinct spiral arms or other structured features are readily apparent, indicating a general lack of ongoing major mergers or significant star formation across the galaxy's disk. The overall morphology suggests a system that has largely undergone its major evolutionary processes, settling into a more quiescent state. There are subtle indications of minor disturbances that may be due to smaller mergers. The galaxy appears nearly circular, showing only slight elongation.
