The galaxy presents a generally smooth, elliptical morphology. It appears to be largely spheroidal with a high degree of central concentration, showing a dominant bulge component. There is a subtle elongation, though the galaxy is generally roundish in overall form. No distinct spiral arms or prominent dust lanes are discernible within the resolution of the image. The color is dominated by reddish-yellow hues, suggesting a population of older, cooler stars, consistent with a low star formation rate. There is no evidence of active galactic nuclei features, tidal tails, or other major disturbances indicative of recent merger activity. Subtle irregularities and blue tinges are visible in the outer edges, which indicates there may be some minor star forming regions present. 
