The galaxy presents as a spiral with a relatively bright, moderately sized bulge. The spiral arms appear somewhat tightly wound around the central bulge. While the image resolution is limited, there is indication of two primary spiral arms. The galaxy exhibits a slight elongation, suggesting the possible presence of a bar structure. The color profile indicates a relatively high concentration of older stellar populations within the bulge, transitioning to bluer, star-forming regions within the arms. There does not appear to be any significant tidal disturbances or obvious signs of ongoing major merger events. However, a slight asymmetry in the arm structure hints at a potential minor interaction or internal dynamic process.
