The observed galaxy presents as a roughly elliptical structure with a notable central bulge. The color distribution suggests the presence of varying stellar populations. The core region exhibits a yellow-greenish hue, potentially indicating older stars or significant dust obscuration. Surrounding the central bulge, a bluer, more diffuse halo is observed, possibly indicative of younger, hotter stars or ongoing star formation. The overall shape suggests the galaxy is an early type spiral that appears more elliptical due to its angle of observation or age, and shows signs of disruption. Faint features are present at the center, possible indications of minor disturbances, such as interactions or internal processes. There appears to be a prominent dust lane across the center of the galaxy.
