The galaxy presents as a largely smooth, elliptical morphology with a concentrated central bulge. The light profile exhibits a high degree of radial symmetry. A slight color gradient is observed, transitioning from a more yellow-orange hue in the central region to a slightly redder color towards the outer edges. There is no apparent spiral arm structure, disk-like feature or active star formation regions that I can see. Based on the red color and smooth morphology, this galaxy may have a population of older stars and a relatively low star formation rate. There is no evidence of any major tidal disturbances or ongoing mergers.
