The galaxy presents as a generally smooth and rounded structure. There is little to no indication of spiral arms or a prominent disk. The galaxy exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. A slight elongation is present, deviating from a perfectly circular shape. No significant tidal features or signs of ongoing mergers are readily apparent. Based on the overall morphology, this galaxy likely represents an elliptical or lenticular galaxy at an approximate distance corresponding to a redshift of roughly 0.2. Its color index suggests a population of older stars, consistent with a relatively low rate of star formation.
