The galaxy presents a somewhat elongated, disk-like morphology, but it does not appear to be strictly edge-on. The central region exhibits a concentration of light, appearing yellowish-white, suggesting an older stellar population. Moving outward from the center, the galaxy transitions to a bluish hue, particularly on what appears to be the outer edges of the disk. This may indicate the presence of younger, hotter stars in these regions.

The disk appears somewhat disturbed or uneven, hinting at possible minor interactions or internal activity. There's no distinct spiral arm structure readily apparent, although some irregularities in the light distribution suggest non-uniform density within the disk. Overall, the galaxy exhibits characteristics of both smooth and featured morphologies. No strong tidal tails or obvious signs of a major merger are visible, though subtle asymmetries indicate potential minor disturbances.
