The galaxy presents a generally smooth and rounded morphology. It appears as a single, cohesive structure with no readily discernible spiral arms or bar. The light distribution suggests a centrally concentrated luminosity profile. The core of the galaxy exhibits a yellowish hue, possibly indicative of an older stellar population. The outer regions display a slightly bluer tint, hinting at the presence of younger stars or ongoing star formation activity, albeit at a low rate. There is no evident signs of tidal disturbances, major mergers, or significant asymmetries in its shape, suggesting that it is a relatively undisturbed system. The overall structure appears to be elliptical or lenticular in nature.
