The galaxy presents a generally smooth, elliptical morphology. The light profile exhibits a strong central concentration, suggesting a prominent bulge component. The galaxy appears nearly circular in projection, with no obvious bar or spiral arm structures visible. A color gradient is present, with the central region exhibiting a yellowish hue, possibly indicating an older stellar population. Fainter, bluer light extends outwards from the core, hinting at the presence of a younger stellar population at larger radii, though the overall star formation rate is likely low. There is no clear evidence of any ongoing major merger activity or significant tidal disturbances, although very minor irregularities cannot be ruled out. The galaxy appears to be a relatively undisturbed system, consistent with a classification as an early-type galaxy.
