The galaxy presents as a moderately luminous, elliptical morphology. Its overall color is dominated by older stellar populations, appearing yellow-orange. The light distribution is centrally concentrated, decreasing gradually towards the outer regions. There appears to be a slight elongation along one axis, giving it a somewhat cigar-shaped appearance. There is minimal evidence of spiral arm structure or significant dust lanes. No obvious signs of active galactic nuclei or recent merger events are apparent, though a minor disturbance cannot be ruled out. The galaxy appears relatively smooth in texture, lacking strong features or substructure. The estimated physical size of the galaxy is approximately 10.5 kpc. Based on the color and morphology, star formation activity appears to be present, but likely at a modest rate.
