The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a concentrated central bulge which is the brightest region of the galaxy. Moving outward from the center, the intensity of light decreases gradually. The overall shape is slightly elongated, approaching a cigar-like appearance rather than being perfectly spherical. No distinct spiral arms or prominent dust lanes are discernible, suggesting a lack of significant ongoing star formation. The galaxy's color is generally redder, indicative of an older stellar population. No apparent merger activity or significant disturbances in the morphology are evident in the image.
