The galaxy exhibits a distinct spiral structure with tightly wound arms. The galaxy's disk appears to be moderately inclined relative to our line of sight. A prominent bulge is observed, occupying a significant portion of the galaxy's central region. The galaxy's color suggests a mixture of stellar populations, with a slightly more yellowed central bulge indicative of older stars and a somewhat bluer disk containing younger stars. There appears to be a slight asymmetry in the arm structure, suggesting a potential past interaction. Star formation is less apparent as there are fewer areas of intense blue color typically associated with star forming regions. The galaxy's light is strongly concentrated and is elliptical in shape.
