The galaxy presents as a relatively small, edge-on spiral system. A distinct central bulge is observed, appearing noticeably bright with a yellowish hue, indicative of an older stellar population. This bulge seems to be round, not boxy. The disk is thin and elongated, obscuring much of its internal structure. Dust lanes are not clearly visible, but there's a slight dimming of the galaxy's light near the edges of the disk, suggesting some dust presence. The disk appears to be composed mostly of older stars. The galaxy appears undisturbed, without obvious signs of recent merger activity or tidal distortions. Star formation activity seems low, based on the absence of bright blue regions or HII regions within the visible disk.
