The galaxy exhibits a centrally concentrated morphology with a relatively smooth appearance. The core region appears bright and yellowish, suggesting a population of older stars. The outer regions show a slightly bluer hue, possibly indicating a younger stellar population or ongoing star formation, albeit at a modest rate. The galaxy's shape appears somewhat elliptical, with a slight elongation visible. There is no strong evidence of spiral arm structures or major disturbances. Faint, diffuse light extends outwards from the core, gradually fading into the background. 
