The galaxy presents as a slightly elliptical structure, with a relatively smooth light distribution. There appears to be a bright central region that gradually fades into the surrounding disk. The galaxy exhibits a subtle color gradient; its core appears more blue-ish, suggesting the presence of younger, hotter stars or potentially an active galactic nucleus. A faint, reddish area is also visible. There are no readily apparent spiral arms, bars, or other distinct morphological features typically associated with late-type galaxies. The galaxy appears relatively undisturbed.
