The galaxy presents as a somewhat elliptical, luminous spheroid with a high degree of central concentration. The core exhibits a bright, almost unresolved appearance, suggesting a significant stellar density or perhaps an active galactic nucleus. The overall color is yellowish, indicative of an older stellar population dominated by redder, evolved stars. There is little evidence of spiral arm structure, suggesting a relatively smooth stellar distribution. Minimal dust lanes or patchy regions of star formation are visible, corroborating the interpretation of an older, more quiescent system. The absence of prominent blue regions further supports the conclusion that ongoing star formation is limited. The galaxy appears relatively isolated, with no obvious tidal features or close companion galaxies that would indicate recent or ongoing mergers. Its shape is very close to circular.
