The galaxy presents a roughly elliptical morphology. Its central region exhibits a bright, concentrated core, likely indicative of a significant stellar population density or possible active galactic nucleus. The color distribution suggests the core may consist primarily of older stars.

Extending outward from the core is a fainter, more diffuse disk. There is some indication of internal structure within the disk, potentially spiral arms. The bluer color of these regions suggests younger star formation. There is no evidence of ongoing major mergers or interactions, however some minor disturbance may be occurring.
