The galaxy presents a somewhat elliptical morphology, with a higher concentration of luminosity toward the central region. The core exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, a subtle blueish tint becomes apparent, possibly indicating the presence of younger, hotter stars within the galaxy's spiral arms or disk-like structure. The overall structure appears relatively smooth with some indications of disruption, but there are signs of faint, extended features or tidal tails, hinting at possible gravitational interactions or a past merger event.
