The galaxy presents a relatively smooth and rounded morphology, appearing largely featureless at this resolution. A central, bright region is evident, suggesting a concentration of stellar mass or an active galactic nucleus. The colour gradient shows a yellowish-white core fading to a faint blueish halo. The halo suggests a distribution of older stars or a low-level star formation rate. There is no clear evidence of spiral arms, bars, or significant tidal disturbances indicating the absence of a major merger event. The galaxy seems to be a relatively isolated, well-formed elliptical or lenticular type.
