The galaxy presents a generally smooth and elliptical morphology. There is a concentrated central bulge with decreasing luminosity outwards. The isophotes are generally elliptical in shape, appearing somewhat elongated, and the galaxy does not exhibit any distinct spiral arm structure or prominent dust lanes. There is no apparent evidence of ongoing major merger activity or tidal disturbances. The galaxy's color appears relatively uniform across its extent, trending slightly towards redder hues. There is a subtle indication of blue color. It may indicate a very low level of star formation.
