This galaxy presents as an elongated, somewhat cigar-shaped structure. The central region exhibits a concentrated luminosity, appearing predominantly orange-red, suggesting a population of older stars and potentially significant dust obscuration. Moving outward from the core, a subtle color gradient is observed. The outer regions display a slightly bluer hue, indicative of younger stellar populations and possibly ongoing star formation. The galaxy appears relatively smooth in overall texture, with no obvious spiral arm structures or major morphological disturbances. The light distribution is largely symmetrical.
