The galaxy presents a generally smooth morphology with a notable elongation, appearing cigar-shaped. There is a concentration of light towards the center, indicating a bulge or a bright nucleus. The color gradient transitions from a yellowish hue in the central regions to a slightly bluer tinge at the outer edges, possibly suggestive of ongoing star formation activity in the disk. No obvious spiral arm structures are visible. There appears to be a subtle distortion or a minor disturbance in the galaxy's shape, but no clear signs of a major merger event are apparent.
