The galaxy presents as a slightly elongated, centrally concentrated object. The core exhibits a bright, whitish-yellow hue, suggesting a population of older stars and/or the presence of an active galactic nucleus. The galaxy gradually fades out into a more diffuse halo. The outer regions display a faint, bluish tint, which could indicate the presence of younger, hotter stars, hinting at ongoing or recent star formation, albeit at a relatively low level. There appears to be minimal evidence of strong spiral arms or a well-defined disk structure; the overall morphology is smooth and relatively featureless. There is some distortion, potentially indicating minor gravitational interactions with another galaxy.
