This galaxy presents a moderately elongated morphology, appearing as a flattened disk viewed at an angle. The color distribution suggests a central concentration of older stellar populations, exhibiting a yellowish-gold hue, indicative of evolved stars. Fainter blue patches are observed, potentially regions of ongoing star formation. These areas are less distinct, possibly due to the galaxy's distance and resolution limitations. The overall structure appears relatively smooth, with no pronounced spiral arms immediately visible. Based on its apparent smoothness and disk-like appearance, it may be a lenticular or spiral galaxy seen at a significant distance. There appears to be some disturbance in the disc.
