The galaxy presents an approximately elliptical morphology, appearing moderately smooth with subtle features. The light distribution suggests a concentration of stars towards the galactic center, with a gradual decrease in intensity outwards. The color profile indicates a dominant population of older stars, exhibiting a reddish hue in the outskirts and trending towards a more bluish color at the core, suggestive of recent or ongoing star formation. There appears to be some disturbance in the light profile, indicating a potential interaction or merger with another galaxy. Overall, the galaxy shows characteristics of late type system with some possible disturbances.
