The galaxy presents an elliptical morphology, appearing largely spheroidal with a smooth, diffuse light distribution. The core exhibits a bright, concentrated luminosity, gradually fading towards the outer regions. The color profile indicates a dominant yellowish-orange hue in the central region, which could suggest an older stellar population. Faint bluish tones are visible in the outskirts, possibly indicating some presence of younger, bluer stars or regions of ongoing star formation. There's no apparent spiral arm structure or significant dust lane obscuration detectable in the image. There is no evidence of tidal tails or other major disturbances that would suggest a recent galaxy merger, however, some minor unevenness might be present.
