The galaxy presents an overall smooth morphology, with a central bulge that appears relatively bright and concentrated. The galaxy's shape is elongated, appearing more cigar-shaped than circular. There is evidence of a faint, diffuse disk component extending beyond the central bulge. This disk shows signs of slight disturbance, potentially due to minor gravitational interactions or internal processes. The color of the galaxy suggests a moderate amount of star formation activity. The central bulge exhibits a yellowish hue, indicative of an older stellar population, while the disk shows some bluer regions, pointing to ongoing star formation. The galaxy does not appear to be undergoing a major merger.
