The galaxy presents as a somewhat elongated structure, suggestive of a spiral or lenticular type seen at a high inclination. There is a bright central bulge that appears relatively smooth.  The disk component exhibits hints of structure, possibly spiral arms, though the resolution and viewing angle make these features indistinct. The galaxy's color is dominated by a yellowish-white hue in the central regions, transitioning to a bluer tint further from the core. This color gradient could indicate a mixed stellar population, with older, redder stars concentrated in the bulge and younger, bluer stars in the disk. Patches of nebulosity may exist within the disk, implied by the bluer, irregular regions. Overall, the galaxy appears to be relatively quiescent, with potentially moderate ongoing star formation. There are no obvious signs of a major merger event.
