The galaxy presents an ellipsoidal morphology with a smooth light distribution, suggesting an elliptical or lenticular classification. The galaxy exhibits a centrally concentrated bulge, contributing significantly to its overall luminosity. The color profile is predominantly red/yellow, indicating an older stellar population with relatively low levels of ongoing star formation. Evident signs of a possible ongoing merger or tidal interactions can be seen in the outer regions of the galaxy; further analysis is needed to confirm the classification. Based on the morphology and color indices, the galaxy is likely a mature system with a substantial stellar mass.
