The galaxy presents as a somewhat diffuse and elongated structure. It appears primarily smooth in overall texture, with a subtle central concentration of luminosity that may indicate a bulge. There is some evidence of disturbance in the galaxy’s morphology. The primary body of the galaxy may be undergoing a merging event with a smaller structure, causing irregularities in the distribution of light. A faint halo or tidal feature may be present. The galaxy exhibits a color gradient, with a bluer hue in the outer regions potentially indicating ongoing star formation and a slightly redder central region. The galaxy lacks a clear spiral arm structure.
