The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. There is a general lack of readily identifiable features, such as spiral arms or a distinct central bar. The light distribution appears to be centrally concentrated, with a gradual decrease in intensity outwards. The object displays a dominant color, suggesting a stellar population composed primarily of older, redder stars, with very low star formation activity. There is a subtle color variation across the galaxy's surface, with a slightly bluer hue concentrated in the galaxy's nucleus. There is no obvious evidence of recent major mergers or tidal disturbances, however there is some indication of minor interactions. The galaxy is fairly rounded in appearance, with an axial ratio close to unity.
