The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish core, possibly indicative of an older stellar population. There is a subtle extension of fainter, bluer light surrounding the core, suggesting the presence of a more dispersed disk component or potentially a small amount of recent star formation. There is no obvious spiral structure, although minor disturbances are apparent, hinting at a possible past interaction or minor merging event. Overall the galaxy appears relatively isolated.
