The galaxy presents as a relatively smooth, centralized structure with a moderate degree of ellipticity. The core region exhibits a concentrated luminosity gradient, appearing significantly brighter and characterized by a yellowish-orange hue, suggestive of an older stellar population dominating the central mass. Progressing outward from the core, a gradual decrease in surface brightness is observed, transitioning to a bluish halo. While it is largely smooth, there is some subtle irregularity, possibly indicative of faint, unresolved spiral arms or tidal features. The lack of significant morphological disturbances suggests a relatively settled state, with the possibility of minor interactions evidenced by subtle asymmetric features. The overall color profile indicates a mixed stellar population, with older stars in the core and relatively younger stars in the outer regions contributing to the galaxy's spectral energy distribution.
