The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless appearance with no discernible spiral arms or bar structures. The light distribution suggests a centrally concentrated bulge, appearing as a bright, slightly elongated core. The overall color profile indicates a dominant older stellar population, inferred from the redder hue of the bulge region. The outer regions gradually fade into the background, showing a diffuse halo extending beyond the central bulge, which also appears slightly more blue. The shape is largely in between that of a cigar and round galaxy, but is significantly closer to round. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The galaxy is largely settled with only minor signs of disturbances.
