The galaxy presents as a largely featureless, elliptical-like structure with a concentrated central bulge. The color profile exhibits a dominance of redder hues, with a central region that is significantly more luminous, transitioning to a gradual decrease in brightness towards the outer edges. No distinct spiral arms or prominent dust lanes are discernible. The overall smooth morphology suggests a relatively evolved system, potentially with a quiescent star formation rate. The galaxy appears quite round. There are no indications of any ongoing major merging events or significant tidal disturbances visible in the image.
