The galaxy presents an elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. Its overall shape is notably rounded. The central bulge exhibits a bright, concentrated core, surrounded by a more diffuse halo. The color gradient suggests a dominant population of older stars within the bulge, as indicated by the yellowish hue, while bluer tones in the outer regions may indicate the presence of some younger stellar populations. There is no strong indication of significant ongoing star formation, nor are there noticeable signs of major disturbances or mergers. Overall, this galaxy seems to be a relatively undisturbed and evolved system.
