The galaxy presents as a single, concentrated light source, appearing largely smooth and elliptical in shape. The central region exhibits a yellowish-orange hue, indicating a population of older stars. There is subtle evidence of bluer light surrounding the center, suggesting some ongoing or recent star formation. No distinct spiral arms or bar structures are discernible. There are no obvious signs of ongoing major mergers, although there is a faint irregular shape at its boundary which may indicate minor tidal disturbances or past interactions. Overall, the galaxy's morphology suggests it is an evolved system with a substantial stellar mass and relatively low specific star formation rate.
