The galaxy presents a primarily smooth and elliptical morphology. A concentrated central bulge is visible, emitting strongly in the yellow-green wavelengths, suggesting an older stellar population with minimal ongoing star formation. The overall shape appears elongated, somewhere between round and cigar-shaped. A faint, diffuse halo surrounds the central region, exhibiting a redder hue, which could indicate the presence of older, cooler stars in the outer regions of the galaxy. There appears to be no significant signs of a spiral arm structure or strong dust lanes, with minimal indications of merging or major disturbances. The galaxy does exhibit some signs of minor disturbances, which might be the result of earlier interactions. Overall, this is a relatively massive galaxy with low star formation rates.
