The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central region, with a gradual decrease in luminosity towards the outer edges. The core appears yellowish-white, suggesting an older stellar population. The galaxy lacks any prominent spiral arm structure or dust lanes, exhibiting a generally featureless morphology. There is little evidence of active star formation. The overall shape is close to circular. There are no signs of major disturbances, tidal tails, or clear indications of ongoing merger activity. A very faint hint of a possible minor disturbance may be present but is likely inconsequential to the galaxy's primary morphology.
