The galaxy presents as a centrally concentrated, elliptical morphology. Its light profile appears relatively smooth, lacking prominent spiral arm structures or dust lanes. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population, possibly dominated by red giants and other evolved stars. The galaxy's color gradually fades towards its outer edges, suggesting a decrease in stellar density and possibly metallicity with increasing radial distance. The overall shape appears nearly circular, with no significant distortions or tidal features suggestive of recent major merger events. A faint, diffuse halo may be present, extending slightly beyond the main body of the galaxy, but further analysis is needed to confirm its properties and extent. There is a slight indication of a color gradient, with the core appearing redder than the outer regions.