This galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge with a yellowish hue, suggesting a population of older stars. Moving outwards from the center, the galaxy fades into a bluer color. The overall shape appears elongated, but not heavily distorted, indicating that it is not in the process of merging, although some minor disturbances cannot be ruled out. Faint outer regions suggest a gradual decline in stellar density and light intensity. No distinct spiral arms or prominent dust lanes are visible within this image, indicative of a galaxy dominated by an older stellar population with relatively low star formation rate. 
