The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a general yellowish-white hue, suggesting an older stellar population dominating the light output. The core region is noticeably brighter and more intensely yellow than the surrounding disk. A subtle, faint, and bluer component appears to exist in the outer regions of the galaxy, hinting at some presence of younger stars or ongoing star formation, although it doesn't show a spiral pattern. The galaxy appears to be somewhat elongated, with a slight deviation from perfect circularity. No significant tidal disturbances or signs of ongoing major mergers are readily apparent based on visual inspection of the overall structure.
