The galaxy presents a generally smooth morphology, with the light distribution appearing relatively even across its structure. It is elongated in shape, resembling a cigar. There is a subtle suggestion of possible disturbances in its structure but no strong evidence for ongoing major mergers or tidal interactions, although minor interactions cannot be ruled out. The primary body is mostly blue-white, but has subtle variations in color, with possible traces of redder light in the central region. This suggests a more complex stellar population. The bluer component is most likely a result of on-going star formation. Overall, the galaxy appears to be a relatively massive object with a modest rate of star formation.
