The galaxy presents as a relatively compact, disk-like system with a notable bulge. The disk appears moderately inclined with respect to our line of sight. Within the disk, there is faint evidence of spiral arm structure. The overall color appears to be a mix of blue and red hues. There is an indication of some ongoing, although possibly subdued, star formation within the disk, as hinted by the somewhat bluer regions. The bulge appears relatively smooth and more uniformly colored. There is no immediately obvious evidence of any major ongoing mergers or significant tidal disturbances. The galaxy appears to be relatively isolated, without any immediately apparent companion galaxies in close proximity. The apparent size is small, suggesting a relatively distant object.
