The galaxy presents as a slightly elliptical structure with a bright, concentrated central bulge. The disk component appears relatively smooth with faint spiral arm features. There may be some indication of a tidal interaction. This is supported by some asymmetry in the disk and a possible faint structure in the halo on the left side. The color of the bulge indicates an older stellar population, while the disk shows evidence of a younger population and ongoing star formation. The galaxy appears to be relatively massive with a moderate star-formation rate. The overall morphology suggests an intermediate-type spiral galaxy undergoing some form of interaction.
