The galaxy presents as a spiral type, viewed at a significant angle relative to our line of sight. A prominent central bulge dominates the galaxy's core, exhibiting a yellowish hue indicative of an older stellar population. Emerging from the central region are two tightly wound spiral arms, only one of which is readily apparent from the viewing angle. These arms are traced by regions of bluer light, suggesting ongoing star formation activity. The disk appears relatively smooth, without evidence of major tidal disturbances or ongoing mergers. A weak bar structure is suggested, though not distinctly visible. The spiral arms display a medium winding pattern, neither tightly coiled nor exceptionally open. Overall, the galaxy exhibits characteristics consistent with an isolated system undergoing normal spiral arm development.
