The galaxy presents a generally smooth morphology. It has an elongated shape, appearing cigar-shaped, but trending towards being in-between round and cigar-shaped, suggesting an elliptical classification or a lenticular galaxy viewed at an angle. There is a notable color gradient, with the central region exhibiting a yellowish-orange hue that transitions to a bluer periphery. The central bulge appears to be the dominant feature, contributing significantly to the overall luminosity of the galaxy. Faint extensions or tidal features are not readily apparent, indicating either a lack of significant recent interactions or that such features are below the detection threshold. There is no discernible spiral arm structure. The light distribution suggests a relatively old stellar population dominating the galaxy's composition. The overall appearance suggests this galaxy is likely a relatively massive system with a suppressed star formation rate.
