The galaxy appears as a relatively bright, moderately sized object. It displays a predominantly smooth morphology with a possible slight elongation, with the shape classified as somewhere between round and elongated. There is a suggestion of a faint, disturbed disk. The central region is the most luminous, with a color gradient towards slightly redder hues in the outer regions. There are very faint and small arm-like structures visible. The galaxy exhibits a low star formation rate and has a high mass. A likely classification is an early-type spiral galaxy with a prominent bulge, or an elliptical galaxy with residual disk features. There does not appear to be a currently ongoing major merger, but signs of minor interactions or past disturbances cannot be ruled out.
