This galaxy exhibits a roughly elliptical morphology, with a central bright core that diminishes gradually outward. The central region shows a concentration of light, appearing almost spheroidal.

The colour distribution shows a radial gradient. The central core is observed to be a bluer in colour, likely indicating the presence of younger stellar populations or a higher rate of active star formation. Moving outward from the core, the colour transitions toward redder hues, potentially indicative of older stellar populations.

There are some subtle asymmetries in the outer regions of the galaxy, but no clear evidence of a major merger is immediately obvious. The presence of some disturbance cannot be ruled out. 
