The galaxy presents as a relatively smooth, elliptical structure. Its shape deviates slightly from perfectly circular, exhibiting a moderate elongation along a major axis. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue concentrated towards the galaxy's core. There is little evidence of significant dust lanes or spiral arm structures. Marginal disturbances can not be ruled out, however the galaxy's morphology indicates that is likely not currently undergoing a major merger event. The galaxy is relatively compact, with light smoothly concentrated towards the center with no clear knots of star forming regions. Overall, the galaxy appears to be a relatively undisturbed, mature system with a diminished rate of star formation.
