The galaxy presents as a relatively elongated, cigar-shaped structure. A central bulge is subtly discernible, appearing yellowish in color, suggesting an older stellar population. The disk is noticeably flatter and extends beyond the bulge, showing a smoother, more diffuse profile. There are some bluer regions within the disk, hinting at ongoing star formation activity, but it appears to be less prominent overall. The galaxy exhibits a generally undisturbed morphology, with no apparent signs of major merger events or significant tidal features. There are no prominent dust lanes or spiral arm structures readily apparent.
