The galaxy presents as a largely featureless, elliptical-like structure. The light profile appears smooth and concentrated, with a central bulge that dominates the overall luminosity. The color gradient suggests a population of older stars, indicated by the reddish-yellow hue, particularly concentrated towards the galactic core. There is no discernible spiral arm structure or prominent dust lanes within the galaxy's morphology. The shape is close to round, only slightly departing from a perfect circular form. There are no indications of significant tidal disturbances or ongoing major merger activity within the observable structure. The galaxy appears relatively isolated, exhibiting no obvious interactions with neighboring galaxies.
