The galaxy presents as a concentrated, elliptical-like structure with a smooth, even light distribution. Its color is a pronounced yellow-orange hue, suggesting an older stellar population. The high central concentration of light indicates a prominent bulge. There is no visible evidence of spiral arms or significant dust lanes. Faint, diffuse outer regions extend from the central core, gradually fading into the background sky. The overall appearance is of a relatively quiescent, evolved system. No significant tidal features or signs of recent merger activity are apparent.
