The galaxy presents as a centrally concentrated object with an elliptical morphology. Its core exhibits a high degree of luminosity with a reddish-orange hue, potentially indicating an older stellar population or significant dust obscuration. Proceeding outwards, the luminosity gradually decreases, with a diffuse halo region surrounding the central bulge. There is faint blue light visible, indicating some star formation is occurring, but this is not a spiral galaxy. There does not appear to be any major morphological disturbance or merging activity, although a slight asymmetry is present in the outer regions. This could be a residual effect of an interaction, or simply internal variations in the distribution of matter.
