The galaxy presents as a lenticular or early-type spiral system, with an estimated redshift of approximately 0.2025. It exhibits a smooth, elliptical morphology, appearing elongated with an aspect ratio of roughly 3:1. The galaxy’s central region displays a concentrated, luminous bulge, possibly indicative of an older stellar population. Colors are yellowish-white at the core, shifting to a duller red in the outskirts, suggesting a decline in active star formation. No significant signs of spiral arms, dust lanes, or tidal disturbances are observed, implying a relatively undisturbed evolutionary history and the absence of recent major mergers. A very low rate of on going star formation is indicated by the colors and morphology, with a dominant population of older stars. The overall structure appears quiescent, with the galaxy residing within a relatively isolated environment.