The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its shape is predominantly round, with a slight deviation towards an elliptical form. There is no indication of a strong disk presence, spiral arm structure, or significant tidal disturbances indicative of ongoing major mergers. The galaxy exhibits a color gradient, transitioning from a reddish hue in the central region to a slightly bluer periphery. This color profile potentially indicates an older stellar population concentrated towards the galactic core. The light is not particularly strong, indicating a lower rate of star formation. No active galactic nucleus or other signs of intense activity are apparent in the image.
