The galaxy presents as a centrally concentrated elliptical morphology. The core region exhibits a bright, luminous glow, indicating a high density of stars and potentially an active galactic nucleus. Moving outwards from the core, the light profile gradually decreases, suggesting a smooth transition in stellar density. There are subtle indications of a disk structure, but the dominant feature remains the spheroidal shape. The galaxy exhibits a redder hue, with faint spiral arms, and a noticeable lack of prominent dust lanes. There is a subtle blue shift in its outer regions. The outer edges are not sharply defined but gradually fade into the background sky, suggesting a halo of more sparsely distributed stars. The overall appearance suggests a relatively evolved galaxy.
