The galaxy appears as a moderately inclined spiral, exhibiting a relatively face-on orientation. The central bulge presents a concentrated luminosity, with a somewhat obscured morphology. Two prominent spiral arms emanate from the central region, with a flocculent structure discernible along their lengths. These arms appear slightly disrupted, hinting at possible gravitational interactions. The overall color of the galaxy suggests a mix of stellar populations. The core exhibits a bluer hue, indicating ongoing star formation, while the outer regions show a more yellowish tint, which may reflect a higher proportion of older, redder stars. There is no evidence of a significant bar structure. There is no obvious indication of recent major merger events, although subtle disturbances are visible in the spiral arm structure.
