The galaxy presents as a moderately inclined, disk-like structure. It exhibits a relatively smooth morphology, though subtle features indicative of a spiral arm structure are present. The central bulge appears elongated, almost cigar shaped. The color distribution suggests the presence of both older stellar populations, indicated by the reddish hues in the bulge, and younger, bluer stars in the disk. There is no evidence of major mergers or tidal disturbances in this image. Minor disturbances may be occurring, but it is difficult to say for sure.
