The galaxy presents as a moderately luminous, elongated structure. Its overall color is a muted bluish-white, indicating a likely mix of stellar populations, including some recent star formation. The central region is noticeably brighter and possesses a yellowish hue, potentially due to a concentration of older stars or dust obscuration. The light distribution suggests an elliptical morphology, although some subtle features are visible. The apparent lack of well-defined spiral arms or a prominent disk implies a relatively smooth and featureless structure. There is slight apparent distortion or possible tidal feature on its outskirts. The galaxy appears to be isolated, showing no immediate signs of interaction with other nearby galaxies, and lacks a strong tidal tail or obvious morphological disruptions, further supporting a lack of recent major mergers.
