The galaxy presents as a moderately luminous, elongated structure, likely an elliptical galaxy or a lenticular galaxy viewed at an angle. The central region exhibits a concentrated, bright, yellowish core, suggesting a significant population of older stars. Moving outward from the core, the light gradually diminishes, forming a smooth, diffuse halo.  There is a subtle color gradient, with the central bulge appearing more yellow than the outer regions, indicating a potential variation in stellar populations or dust content. No distinct spiral arm structures or significant dust lanes are readily apparent. The overall morphology appears relatively undisturbed, with no obvious signs of recent major merger events. Some minor irregularities are visible, but they are not prominent enough to suggest a strong tidal interaction. The galaxy has an estimated half light radius of 6.7 kpc, with a high mass (log10 > 11), and a relatively low star formation rate (log10 < -0.8), with a redshift of 0.255981.
