This galaxy presents as a relatively smooth, elongated structure. The central region exhibits a bright, concentrated light, indicating a substantial bulge component. There is evidence of a disk, although it appears tightly wound and less prominent. The galaxy's color profile suggests a population of older stars. We don't see much evidence of on going star formation activity; it's predominantly redder in color. Overall, the galaxy displays characteristics of a disk galaxy that is in between a round and cigar shape with a strong central bulge.
