This galaxy presents as a spiral type, viewed at an angle that is slightly inclined from edge-on. The disk structure is clearly defined and exhibits a distinct spiral arm morphology. These arms appear somewhat patchy, with regions of greater intensity suggesting areas of active star formation. Blue hues are visible within these spiral arms, which is indicative of the presence of younger, hotter stellar populations. A central bulge is visible, characterized by a smoother texture and a yellowish coloration, hinting at a population of older stars. No significant bar structure appears to be bisecting the bulge region. The galaxy appears relatively undisturbed, exhibiting no major signs of a recent or ongoing merger event, though a minor disturbance cannot be ruled out given the irregular structure of the spiral arms.
