The galaxy presents as a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a bright core that diffuses outward. The overall color appears to be a blend of yellowish-green hues, with a slight tendency toward redder tones in the outer regions. There are no distinct spiral arms or prominent dust lanes visible in this image. The morphology suggests an evolved system, potentially undergoing passive evolution with limited current star formation, which is consistent with the color profile. The galaxy shows a moderate degree of ellipticity. There does not appear to be any evidence of a major merger or strong tidal disturbances.
