The galaxy presents an elongated, cigar-like morphology with a smooth, diffuse light distribution. It appears to be relatively featureless, lacking prominent spiral arms or distinct clumps of star formation. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a bulge. There's a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a more yellowish or white color towards the central bulge. This hints at a potential difference in stellar populations, with younger, bluer stars populating the outer disk and older, redder stars concentrated in the bulge. A very faint hint of a disk-like structure may be present. There are no obvious signs of ongoing merger activity or significant tidal disturbances.
