The galaxy presents as a relatively smooth, elliptical structure. Its shape appears to be somewhere between round and elliptical. There is a noticeable concentration of light towards the center, with a gradual decrease in brightness moving outwards, suggesting a prominent bulge. No distinct spiral arms or bar features are discernible. The color is generally a yellowish-orange hue, indicative of an older stellar population with reduced recent star formation. There is no obvious evidence of any major mergers or significant tidal disturbances in its immediate vicinity.
