The galaxy presents as a relatively smooth, elliptical object. The central region exhibits a concentrated, bright core, possibly indicating the presence of an active galactic nucleus or a dense stellar population. Moving outward from the core, the light intensity gradually decreases, and the color shifts subtly from yellowish-white to a more reddish hue. This suggests a potential age gradient within the galaxy, with older, redder stars dominating the outer regions. There may be faint disturbances in its morphology, such as minor tidal features, suggesting past interactions with other galaxies. While a disk component is difficult to distinguish, the slight ellipticity hints at some degree of rotational support.
