The galaxy presents as an elongated, cigar-shaped structure. A significant portion of the galaxy’s central region exhibits a smooth, centrally concentrated luminosity. The color in this core is a deep red, suggesting a population of older stars and potentially significant dust obscuration. Extending outwards from the core, the galaxy displays fainter, bluer regions. These are concentrated toward the extreme ends. The blue color may indicate younger stellar populations and ongoing star formation activity. The overall structure appears relatively undisturbed, lacking prominent signs of recent major mergers or interactions, however there is possible disruption on the left side. 
