The galaxy presents as a spiral type, viewed at an angle that is approaching face-on but showing some inclination. It has a prominent central bulge exhibiting a yellowish hue, indicative of an older stellar population. Surrounding the bulge is a disk structure, where spiral arms can be discerned. These arms show a bluish color, suggesting the presence of younger, hotter stars and ongoing star formation. There is evidence of a bar-like structure extending through the bulge, which is offset. The galaxy exhibits a moderate degree of central concentration, with the light intensity decreasing gradually from the center towards the outer regions of the disk. The spiral arm structures appear relatively open. There may be some minor disturbances, such as asymmetries in the outer regions of the disk, but the overall morphology suggests a relatively settled state.
