The galaxy presents as a somewhat elongated, cigar-shaped structure. It displays a relatively smooth overall morphology, lacking prominent spiral arms or distinct substructures. The central region appears brighter and slightly more concentrated, suggesting a possible bulge or nucleus. The light distribution across the galaxy shows a gentle gradient, fading from the center outwards. There is subtle color variation; bluer hues are observed in the outer regions, potentially indicating ongoing star formation. The central region shows hints of a redder hue, indicative of an older stellar population. There is no indication of a major merger or significant tidal disruption.
