The galaxy appears as a somewhat diffuse, centrally concentrated object. The light distribution suggests a generally smooth morphology with possibly a very subtle disk-like structure. There may be a slight hint of spiral arms, but any such features are faint and not well-defined. The central region is bright, potentially indicative of an active galactic nucleus or a dense stellar population. Overall the galaxy seems to be a massive galaxy with moderate to high star formation. There does not appear to be any major merging activity, with the galaxy showing a mostly undisturbed structure.
