The galaxy presents as a somewhat elongated, cigar-shaped structure. It exhibits a smooth morphology with no apparent spiral arms or bar. There's a central bulge that appears to be comprised of older stars, indicated by the redder hue, surrounded by a more diffuse halo extending outwards. This halo region shows a bluer tint, suggesting the presence of younger stellar populations and potentially ongoing star formation, however, the galaxy's overall star formation rate appears to be relatively low. There is no indication of a major merging event.
