The galaxy presents as a somewhat elongated structure, appearing to be an elliptical or lenticular galaxy viewed at an oblique angle. The central bulge is prominent and exhibits a yellowish-orange hue, suggesting a population of older stars. The overall color gradient suggests a transition to bluer hues in the outer regions, potentially indicating the presence of younger stellar populations, although this could also be due to dust attenuation. The smooth appearance dominates, with little discernible substructure or spiral arm features. There is no apparent major disruption or merging activity, although a minor tidal disturbance cannot be entirely ruled out based on the slight asymmetry in the outskirts. The galaxy's moderate size, combined with its redshift, implies a significant distance and luminosity. Star formation activity appears to be low to moderate.
