The galaxy presents as a relatively smooth, elongated structure. Its overall shape is reminiscent of a cigar, with a noticeable central bulge that appears brighter and more concentrated than its outer regions. The color distribution indicates that it is a mix of yellow and red colors with some green areas near the halo, possibly pointing to a significant population of older stars with low star formation in the yellow and red areas. The smooth appearance implies a lack of significant dust lanes or spiral arm structures. There is no evidence of ongoing major mergers or significant tidal disturbances. The galaxy's morphology suggests a relatively evolved system, consistent with an elliptical or lenticular classification.
