The galaxy appears to be a relatively compact object. It exhibits a core region of high surface brightness, which graduates into a somewhat fainter, diffuse halo. The colors within the galaxy are not uniform. The central region displays a bluer hue, indicative of younger stellar populations or higher metallicity gas. Moving outward, the halo becomes progressively redder, suggesting an older stellar population. There is a very faint hint of disturbed morphology or perhaps tidal features in the outer reaches, indicative of possible past interactions, though these are quite subtle. The galaxy lacks any obvious spiral arm structure, though the resolution of the image makes it difficult to definitively rule it out. Overall the galaxy shows characteristics of a smooth morphology, however, this may be due to the resolution of the image. 