The galaxy presents as a relatively smooth, centrally concentrated object with a primarily elliptical morphology. A notable bulge component is observed, exhibiting a warmer color profile suggestive of an older stellar population. Fainter, cooler emission surrounds the central bulge, indicative of a disk or extended halo. There is little evidence of strong spiral arm structures, grand design features, or significant dust lane obscuration. The galaxy exhibits a moderate degree of roundness, showing only slight elongation. No major signs of tidal disturbances or ongoing mergers are immediately apparent, though the faint outer halo could potentially show signs of minor interaction. Overall, the galaxy appears to be an early-type spiral or lenticular galaxy undergoing relatively quiescent star formation.
