The galaxy presents as a spiral type, viewed at an angle slightly off from face-on. The central bulge appears prominent and moderately sized. The disk surrounding the bulge exhibits a complex structure, with indications of spiral arms. These arms are not tightly wound but rather appear more open and less defined. The color distribution suggests a mix of stellar populations, with the bulge exhibiting a yellowish hue, indicative of older stars, and some bluer patches within the disk, possibly signifying regions of more recent star formation. There may be a bar-like feature crossing the central region. There is no evidence of a major merging event. The galaxy exhibits a moderate degree of internal structure.
