The galaxy presents as a barred spiral galaxy with a moderate bulge. The bar structure is prominent and extends across a significant portion of the galaxy's central region. Spiral arms are clearly visible, emanating from the ends of the bar, though their structure appears somewhat flocculent and not tightly wound. Dust lanes are apparent within the spiral arms, obscuring some of the starlight. The bulge exhibits an intermediate size relative to the overall galaxy disk, and is characterized by a smooth, diffuse light distribution. Overall, the galaxy appears largely undisturbed, showing only slight asymmetries that may suggest minor gravitational interactions or past merger events, but no significant tidal features are obvious. The overall color profile indicates a presence of both older stellar populations in the bulge and younger, bluer stars associated with the spiral arms.
