The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical, with a gradual decrease in luminosity moving outward from the core. The color profile suggests a dominant population of older stars, giving it a yellowish-red hue in the central regions. There is a hint of bluer light surrounding the central bulge, implying the presence of some younger, hotter stars or regions of ongoing star formation in the outer regions of the galaxy. The structure appears largely undisturbed, without obvious signs of a major merger or significant tidal interactions. There might be a very slight asymmetry in the outer regions which could be the result of a minor merger.
