The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth morphology with no apparent spiral arm structure. The central bulge is prominent and diffuse, displaying a yellow-orange hue, suggestive of an older stellar population. The isophotes appear somewhat elongated, trending towards a cigar shape, but with deviations from perfect elliptical symmetry. There are no readily apparent signs of significant ongoing merger activity or major tidal disturbances, though a minor asymmetry in the outer regions cannot be ruled out. Overall, the galaxy appears to be relatively evolved with a suppressed star formation rate and high mass.
