The galaxy appears to be a spiral galaxy, seen at a significant inclination relative to our line of sight. It is characterized by a bright, concentrated central bulge that dominates the overall light profile. Extending from the bulge are faint, diffuse spiral arms. These arms seem somewhat fragmented and lack strong definition, which suggests a relatively smooth distribution of stars, with a small portion of clumpy star formation regions. The overall color of the galaxy appears to be on the redder side with some bluer regions indicating ongoing star formation. The galaxy appears isolated, with no obvious signs of tidal interactions or ongoing mergers.
