The galaxy presents as a relatively smooth, elliptical-shaped object. It exhibits a pronounced central bulge with a yellow-orange hue, suggesting an older stellar population and a lack of ongoing star formation within the core. The galaxy's overall color gradient shifts towards redder tones in the outer regions, indicative of a population of aging stars. A slight disk-like structure is present, but the galaxy is largely smooth and lacks prominent spiral arms or significant dust lanes. The major axis is more extended than the minor axis, creating a cigar-shaped appearance. There is no evidence of significant mergers or major tidal disturbances. The galaxy appears undisturbed and relatively isolated.
