The galaxy presents as a centrally concentrated object with a generally smooth appearance. It appears largely elliptical in shape, exhibiting a high degree of circularity. The core region displays a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color shifts slightly towards redder tones, indicating a potential decrease in younger, bluer stars in the outer regions. A faint, diffuse halo surrounds the central region, with a hint of extended structure on one side, though this could be due to interaction, dust, or potentially an artifact of the observation. There's no strong evidence of prominent spiral arms or a distinct disk component. The overall color profile suggests a relatively low rate of star formation. The galaxy does not appear to be undergoing any major merger activity, with no obvious signs of tidal tails or significant disturbances in its morphology.
