The galaxy presents a largely smooth, elliptical morphology. The light profile is centrally concentrated, with a bright, yellowish core that likely indicates an older stellar population. Moving outward from the center, the color transitions to a bluer hue. The edges of the galaxy appear somewhat diffuse, lacking sharp definition and indicating a gradual fading of stellar density with increasing radius. There is no clear evidence of spiral arms or a prominent disk structure within the galaxy's overall shape. The galaxy appears relatively undisturbed, with no obvious signs of recent or ongoing major mergers or tidal interactions with other galaxies. It exhibits a near-circular appearance, with only a very slight deviation from perfect roundness. There appears to be weak star formation occurring.