The galaxy presents as a relatively smooth, elliptical-like structure with a somewhat round morphology. It exhibits a dominant bulge component, indicated by a concentration of light towards the center. The color profile suggests a population of older stars, seen from the reddish and green hues, though there appears to be ongoing star formation activity in the center of the galaxy. There are no distinct spiral arms or a prominent disk structure visible, and there are no indications of any major merger events or significant tidal disturbances affecting the galaxy’s overall form. The color distribution is fairly uniform across the galaxy, with a slight increase in red color towards the central region. The galaxy appears to be relatively isolated.
