The galaxy presents a generally smooth morphology, appearing largely elliptical in shape, though with a slight departure from perfect sphericity. The light distribution suggests a concentrated central bulge that fades gradually outward. There is little evidence of spiral arm structure or distinct features typically associated with disk galaxies. The color appears to be predominantly yellowish-orange, consistent with an older stellar population and lower ongoing star formation. Subtle irregularities in the outer regions may suggest past minor gravitational interactions. The estimated size of the galaxy is on the order of a few kiloparsecs.
