This galaxy appears to be a spiral galaxy, presenting an edge-on or highly inclined view from our perspective. The central bulge appears prominent and somewhat elongated. Faint, diffuse arms are visible extending from the central region. There is a noticeable blueish hue in these outer regions, likely indicating the presence of younger, hotter stars and ongoing star formation within the spiral arms. There appears to be a possible dwarf galaxy interacting with it as well. There are subtle irregularities in the arm structure, suggesting possible gravitational interactions with a smaller companion or past merger events.
