The galaxy presents as a smooth, elliptical-like object with an elongated morphology. The central region exhibits a high concentration of light, appearing bright and yellowish-white. Moving outwards, the light gradually diffuses into a fainter halo. The galaxy appears undisturbed with no obvious signs of ongoing merging activity or major tidal disruptions. There may be slight evidence of a disk, but the smoothness of the overall light distribution strongly suggests a dominant bulge component. There are no distinct spiral arms or prominent dust lanes visible in this image. The galaxy appears reddish in color, implying an older stellar population and moderate to low levels of star formation.
