The galaxy presents as a centrally concentrated object, roughly elliptical in shape, with a smooth light distribution and no readily apparent spiral arm structures or prominent dust lanes. It exhibits a yellowish hue, suggestive of an older stellar population with diminished ongoing star formation. The core region appears brighter and more compact than the outer regions, indicating a possible concentration of older, redder stars or a central supermassive black hole actively accreting matter. There are no clear signs of tidal tails or other significant disturbances in its morphology that would indicate recent major merger events, though some minor asymmetry in the outer regions cannot be ruled out. The galaxy appears relatively isolated and undisturbed.
