The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology, suggesting an early-type classification. It exhibits a moderately round shape with a gradual decline in surface brightness from the core outward. A slight disturbance in its structure is hinted at by subtle asymmetries in the outer regions, possibly indicating a past minor interaction or accretion event. There appears to be a very subtle blue tinged disk. The core displays a yellowish-white hue, transitioning to a slightly bluer color in the outer regions. This color gradient indicates ongoing, although subdued, star formation activity, with a greater proportion of older, redder stellar populations residing within the central bulge. The overall color profile suggests a relatively evolved system, with a moderate stellar mass and low specific star formation rate.
