This galaxy appears to be a spiral galaxy viewed nearly edge-on. The central bulge is bright and elongated, indicating a significant concentration of older stars. A flattened disk extends outwards from the bulge, with a relatively smooth appearance. There is evidence of a dust lane, visible as a dark band obscuring some of the light from the bulge along the galactic plane. Faint hints of spiral arm structure can be seen extending from the bulge, though these are not well-defined. A blue tinge suggests the presence of younger stars. Overall, the galaxy exhibits a moderate degree of internal order, with no significant signs of ongoing major mergers or tidal disturbances.
