The galaxy presents as a slightly elongated spheroid with a concentrated central bulge. The light profile appears smooth and diffuse, lacking any distinct spiral arm structures or prominent dust lanes. The core region exhibits a yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the color gradually transitions to a more bluish tint, suggesting the presence of some younger stars. The overall shape is neither perfectly spherical nor highly elongated, but somewhere in between. No strong signs of tidal disturbances or ongoing mergers are readily apparent, suggesting relative quiescence. Based on the visual morphology, this galaxy is likely a relatively massive system, undergoing modest levels of star formation.
