The galaxy presents a mostly smooth morphology, with approximately 77% of classifications identifying it as smooth. It appears nearly round, but the vast majority of classifications indicate it is somewhere in between round and elliptical. A small percentage show some kind of cigar shape, which indicates ellipticity. There seems to be signs of minor disturbances, with a significant fraction, approximately 46% suggesting a minor interaction or irregularity in its structure. There is evidence of star formation, but at low levels. The galaxy exhibits a yellowish hue in its core, suggesting an older stellar population, and appears somewhat diffuse, with a gradual transition between its central region and outer edges.
