The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge of high luminosity that gradually decreases in intensity toward the outer edges. There is no apparent dust lane, spiral arm structure, or other significant features indicative of active star formation. Its shape appears relatively circular, with a very slight elongation. It shows no visually obvious signs of recent mergers or major disturbances. The light appears to be shifted towards the redder end of the spectrum, which suggests an older stellar population and a relatively low star formation rate. The overall structure implies a well-matured and stable galactic form.
