The galaxy presents as a spiral type with a prominent central bulge, viewed at a tilted angle relative to our line of sight. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Spiral arms emanate from the central region. These arms show a distinct structure, tracing a generally defined two-armed pattern. The winding of the spiral arms appears to be intermediate, neither tightly wound nor loosely dispersed. There is evidence of a bar-like structure traversing the central region of the bulge. The disk appears as a plane containing numerous regions of star formation or dust. The disk shows a bluer color, indicating the presence of younger, hotter stars. The galaxy does not appear to be undergoing any major merging activity, though some minor disturbances may be present in the outer regions of the disk. The size of the bulge appears moderate in comparison to the overall size of the disk.
