The galaxy presents as a luminous, relatively smooth and rounded structure. Its overall color is yellowish, suggesting a population of older stars. There is a slight color gradient toward the center, potentially indicating a higher concentration of older, redder stars in the core. The galaxy exhibits a subtle disk-like morphology, although no distinct spiral arms or prominent features are readily apparent. There is no indication of ongoing major merger activity or significant tidal disturbances. The estimated mass of the galaxy is substantial, with the star formation rate being relatively low. The specific star formation rate suggests the galaxy is not currently undergoing a major burst of star formation.
