The galaxy presents as a moderately luminous, elliptical or lenticular system with a pronounced central bulge. The morphology appears largely smooth, with a general lack of distinct spiral arms or prominent dust lanes. The galaxy exhibits a color gradient, trending from yellow-orange in the central region towards a slightly bluer hue in the outer edges. This suggests a centrally concentrated older stellar population with possibly ongoing, lower-level star formation in the outer regions, which has an estimated size of 3.6 kpc. The overall form is somewhat elongated. There is no strong evidence of active galactic nucleus activity or recent major merger events based on the visual appearance. The galaxy appears relatively undisturbed, with no clear signs of tidal tails or significant morphological distortions.
