This galaxy appears to be a relatively smooth, disk-shaped system with a concentrated central bulge. The bulge exhibits a bright, yellowish-white hue, suggesting a population of older, cooler stars. Moving outward from the bulge, the disk becomes less defined, with a gradual fading of luminosity. The disk material has a slight reddish tint, which could indicate the presence of dust obscuring the view or a population of older stars. The galaxy seems to be elongated, with the major axis considerably longer than the minor axis, suggestive of an edge-on or highly inclined viewing angle. There is little evidence of distinct spiral arms, but some minor irregularities in the disk's outer regions might hint at underlying structures. The overall smooth appearance implies that it might be undergoing limited star formation activity currently. There are no obvious signs of a major merger or significant tidal disturbances.
