The galaxy presents as a slightly inclined spiral, approximately 11.9 kpc in diameter at the widest point. The central bulge exhibits a yellowish hue, suggesting a population of older stars. The disk surrounding the bulge displays a bluer tint, indicative of ongoing star formation activity. The spiral arms are not well-defined, appearing somewhat flocculent and patchy. The overall shape is elliptical, with a ratio of the minor to major axis of approximately 0.79. There are no obvious signs of a major merger event, but some subtle disturbances within the disk may suggest minor interactions.
