The galaxy presents as an elliptical morphology, appearing generally smooth in texture with no readily discernible spiral arms or bar structure. The light distribution exhibits a radial profile, with the brightest concentration towards the core region. The galaxy displays an intermediate degree of ellipticity, tending towards a rounded shape rather than an elongated form. There are no indications of major mergers or significant tidal disturbances influencing its structure. The color profile suggests a generally older stellar population, based on the redder color index. Overall, the system appears to be a relatively quiescent galaxy with characteristics consistent with an evolved stellar population and minimal ongoing star formation.
