This galaxy presents as a disk galaxy seen nearly edge-on from our vantage point. A prominent, centrally located bulge dominates the galaxy's overall form. The bulge exhibits a smooth, rounded structure with a yellowish hue, indicative of an older stellar population. A faint, flattened disk extends outwards from the bulge. Hints of darker dust lanes are visible along the galactic plane, though these are not highly distinct. The disk's color gradients suggest the presence of some ongoing star formation, though at a relatively low rate. There is no strong evidence of a recent or ongoing major merger event, although minor tidal disturbances cannot be ruled out.
