The galaxy presents a largely smooth, elliptical morphology. A concentrated central bulge is apparent, emitting strongly. The color of the bulge appears yellowish-white, suggestive of an older stellar population. A faint, diffuse halo surrounds the central region, extending outwards. This halo exhibits a slightly redder hue, potentially indicating the presence of a population of older, cooler stars or dust. No prominent spiral arm structures or dust lanes are discernible within the visible structure. The overall appearance suggests a relatively evolved galaxy, potentially undergoing low levels of star formation. There is no visual evidence of major recent merger activity, although minor disturbances cannot be ruled out. The galaxy's morphology is largely undisturbed and relaxed.
