The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be elliptical or lenticular, displaying a high degree of circularity. The light distribution is not perfectly uniform, exhibiting a subtle gradient from a bright central region outwards. There is faint evidence of a possible minor tidal disturbance or interaction occurring, indicated by a faint extension of the galaxy's light distribution to its side. The galaxy exhibits a color profile consistent with an older stellar population, with light in redder wavelengths dominating. Overall, the galaxy appears to be a mature system, potentially with suppressed star formation activity.
