The galaxy presents a generally smooth morphology, exhibiting a prolate spheroidal shape. The light is concentrated toward the center of the galaxy, implying a dense galactic nucleus. The observed color gradient suggests a moderate population of older stars, particularly within the central bulge, which displays a more yellow to reddish hue. Fainter, blueish regions surround the primary structure, indicating the presence of some younger, hotter stars, potentially within a faint disk or spiral arms. No signs of a major ongoing merger are visible. There is some minor irregularity in the outer halo regions.
