The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. It appears concentrated, with a significant central bulge that dominates the visual structure. There is a slight elongation, deviating marginally from a perfectly circular form. The color profile is generally redder, with a hint of yellow in the center. This coloration implies an older stellar population, potentially with fewer active regions of star formation. Indications of a disk structure are not readily apparent. There are no obvious signs of tidal tails, bridges, or other pronounced disturbances typically associated with recent major mergers, although subtle irregularities might indicate minor gravitational interactions.
