The galaxy presents as a relatively smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish hue, suggesting an older stellar population. There's a gradual falloff in surface brightness extending outward from the core, transitioning to a bluer color in the outer regions. The overall morphology appears largely elliptical, with no readily apparent spiral arm structure or bar. Subtle irregularities in the outer envelope may indicate minor tidal interactions or recent accretion events, but these are not prominently displayed. Based on its smooth morphology, the galaxy is likely an elliptical galaxy or a lenticular galaxy with a dominant bulge component. The presence of blue light in the outer regions indicates some ongoing star formation.
