The galaxy appears as a slightly elliptical structure with a moderate degree of central concentration. It has an estimated effective radius of approximately 10 kpc. There are some indications of disruption in the galaxy's morphology, potentially due to minor interactions or internal processes. The central region is characterized by a yellowish hue, suggesting the presence of an older stellar population, while some bluer regions are also visible indicating ongoing star formation. Based on the colors, this galaxy is likely massive, with an estimated stellar mass exceeding 10^11 solar masses. Overall, this galaxy is categorized as an early-type spiral with an estimated redshift of z ≈ 0.24.
