The galaxy presents as a spiral type, exhibiting a prominent disk structure viewed at an inclined angle. Observable spiral arms are present, with tightly wound morphology. A central bulge is visible, appearing moderately sized. No significant bar structure is discernible within the central region. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major merger events or significant tidal disruptions. Its color profile shows a mixture of stellar populations with the bulge presenting a yellowish color, possibly indicating an older stellar population. Some blue star forming regions are seen within the spiral arms.
