The galaxy presents as a slightly elongated, diffuse structure with a concentrated central bulge. Its overall color appears to be a yellowish-white, hinting at a population of older stars. There is a faint, bluer halo surrounding the main body, possibly indicating the presence of some younger stellar populations or ongoing star formation. No prominent spiral arms or dust lanes are discernible in this image. The smoothness of the light distribution suggests the galaxy is likely an elliptical or lenticular galaxy, rather than a spiral. The central bulge dominates the light profile, which decreases gradually into the outer regions. There is no apparent sign of a major merger event or significant tidal disturbances. The galaxy exhibits a relatively high degree of central concentration and is moderately large in size.
