The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution without any readily apparent spiral arm structures or distinct features. The core is relatively bright and concentrated, appearing yellowish-white, indicating a likely older stellar population dominating the central region. Moving outward from the center, the light gradually diffuses into a fainter halo. The outer regions show a subtle bluer tint, suggesting the presence of younger, hotter stars, although their contribution to the overall light is minor. The galaxy's shape is slightly elongated, deviating from a perfect circle. It appears to be relatively isolated with no obvious signs of recent major mergers or interactions, although subtle disturbances may be present. The overall color profile suggests the galaxy is relatively quiescent in terms of ongoing star formation, with a lower rate of star formation in the galaxy.
