The galaxy presents as a generally smooth and elliptical-shaped structure, with no apparent spiral arm morphology. It exhibits a concentrated central bulge that appears yellowish-white in color, suggesting an older stellar population. The outer regions of the galaxy appear less luminous and slightly bluer, possibly indicative of a younger stellar population or ongoing star formation at a low rate. The overall color gradient transitions from a warmer hue in the core to cooler tones towards the edge. The galaxy does not display any obvious signs of major mergers or significant tidal disturbances; however, a faint, irregular halo cannot be entirely ruled out given the image resolution. The ellipticity of the galaxy is moderate, indicating that it is viewed at an oblique angle.
