The galaxy appears as a moderately bright, elliptical-shaped object. Its central region exhibits a concentrated, smooth light profile, suggesting a prominent bulge. There's a noticeable decrease in luminosity moving outward from the core towards the edge of the galaxy, indicating a diminishing stellar density. The galaxy's overall color seems yellowish-white, with a subtle hint of red, implying a population of older stars and a relatively low rate of ongoing star formation. There are no distinct spiral arm structures or prominent dust lanes visible in this image. A slight irregularity in the overall shape suggests the possibility of a minor gravitational interaction or disturbance, but there is no single obvious companion galaxy in this image, so any interaction appears to be the result of merging. 
