The galaxy presents a largely spheroidal morphology with high degree of central concentration of light. The luminosity profile suggests a smooth distribution of stars, with a gradual decline in brightness from the core outwards. The galaxy appears nearly circular. There is no apparent spiral arm structure.

The core exhibits a bright, yellowish-white glow, indicative of an older stellar population. The outer regions are dimmer with more reddish hues, potentially due to the presence of older and cooler stars, or dust. The galaxy lacks distinct dust lanes or prominent regions of active star formation.
