The galaxy presents as a spiral with a relatively bright central bulge, suggesting the presence of a supermassive black hole at its core. The spiral arms are prominent but not tightly wound, displaying a more open structure. The arms are slightly asymmetrical, indicating potential gravitational interactions or past minor merger events. The color profile suggests ongoing star formation within the spiral arms, with bluer regions interspersed with more yellow and reddish older stellar populations. No clear evidence of a strong bar feature bisecting the galaxy is apparent. The dust lanes are subtle but discernible within the spiral arms. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disruptions in the immediate vicinity.
