The galaxy exhibits a generally smooth morphology, although subtle features are present. It appears elongated, with an approximate cigar shape, suggesting it may be an elliptical galaxy viewed from an angle. The central region is brighter and displays a yellowish hue, potentially indicating an older stellar population. Fainter, somewhat bluer regions are observed towards the outer edges of the galaxy, suggesting the presence of some younger stars or regions of ongoing star formation. No obvious signs of strong tidal disturbances or major mergers are observed in the immediate vicinity. The overall structure appears relatively undisturbed. The lack of well-defined spiral arms or a prominent disk supports the classification as an elliptical galaxy or a lenticular galaxy.
