The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a notable degree of roundness, lacking any prominent disk-like or cigar-shaped features. There is no clear evidence of ongoing or recent major merger activity, although subtle irregularities suggest the possibility of minor gravitational interactions. The object appears relatively uniform in color, indicating a lack of significant spatial variation in stellar populations or dust content. The overall luminosity suggests a considerable stellar mass. Given the lack of distinct features and smooth light distribution, star formation appears to be relatively quiescent within the galaxy.
