The galaxy presents as a luminous, centrally concentrated object with a slightly elongated shape. The core region exhibits a bright, smooth appearance, suggestive of an older stellar population. There is evidence of a possible ongoing or recent merger event. A notable feature is the presence of a second region of concentrated light a small distance from the center. This may indicate an interaction with a smaller companion galaxy. The overall color profile indicates a range of stellar ages within the system, with a generally redder appearance. This is consistent with a galaxy that may have a moderate rate of star formation. The galaxy's moderate size, based on its angular extent, is consistent with it being a relatively massive system.
