The galaxy appears as a concentrated, elliptical structure. The light profile is centrally concentrated and fades gradually towards the outer regions. The core exhibits a yellowish hue, suggestive of an older stellar population. There is little evidence of spiral arms or distinct disk features. The galaxy exhibits a smooth appearance, lacking prominent dust lanes or active star-forming regions, it displays a moderate red shift, indicating that it is at an intermediate distance. The overall morphology suggests a system undergoing quiescent evolution, potentially a result of an earlier merger.
