The galaxy appears to be relatively compact, with an estimated half-light radius of approximately 3.8 arcseconds. The overall morphology exhibits a somewhat amorphous structure, suggesting either a smooth profile or the presence of disturbed features within a disk. There is no evidence of a strong spiral arm structure, although the image quality may limit the detectability of finer details. The central region is characterized by a bright, concentrated core, surrounded by a more diffuse halo of fainter light. The galaxy displays a subtle color gradient, transitioning from a bluer hue in the inner regions to a slightly redder color in the outer extent. The appearance suggests a possible recent or ongoing interaction, although the limited resolution makes it difficult to determine if the disturbances are a result of a minor merger event. The observed features are faint, and the galaxy appears to be relatively isolated in the field.
