The galaxy presents as a moderately bright, centrally concentrated object with a somewhat diffuse halo. Its morphology appears largely smooth with little discernible structure in the image. The galaxy exhibits a slight elongation, deviating moderately from a perfect circular shape. There is a hint of a potential minor disturbance along its edge, possibly indicative of tidal interactions or recent accretion events. The galaxy displays colors suggesting a population of older stars, with a moderate level of ongoing star formation within its core. The color gradients are subtle, indicating a relatively well-mixed stellar population across the galaxy's observed area.
