The galaxy exhibits a generally smooth morphology, lacking prominent spiral arms or a strong bar structure. The light distribution appears relatively concentrated and centrally-peaked. The galaxy appears elliptical, with an apparently spheroidal shape. The primary light emanating from the galaxy appears to be redder and more yellow, suggesting that the galaxy is primarily composed of older stars, with little ongoing star formation. The light of the galaxy seems to be primarily in the redder spectrum. There may be a possible presence of a minor merger or tidal disturbance, evidenced by slight distortions in the outer regions of the galaxy's isophotes. The overall appearance suggests a relatively evolved system.