The galaxy presents as a centrally concentrated object, exhibiting a generally elliptical morphology. The core region displays a pronounced yellow/orange hue, suggestive of an older stellar population. There appears to be a slight elongation, deviating from a perfectly circular form. Faint hints of possible tidal interactions or minor disturbances are observed in the overall structure, with subtle asymmetries and a possible plume-like extension visible towards the upper portion of the galaxy. Overall, the object is consistent with a relatively massive galaxy with an estimated size of about 8 kpc, where star formation activity is currently suppressed.
