The galaxy presents as a primarily smooth, elliptical-like structure. Its color profile suggests a significant population of older stars, exhibiting a yellow to reddish hue. The apparent lack of prominent dust lanes or spiral arms implies a relatively quiescent state regarding star formation activity. There are no clear signs of ongoing major mergers or significant tidal disturbances, indicating a dynamically relaxed system. The light appears centrally concentrated. The overall morphology indicates this is likely a massive, evolved galaxy with little active star formation.
