The galaxy presents a largely smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The central region exhibits a high degree of concentration, appearing almost spheroidal in shape. There is a gradual decline in surface brightness moving outwards from the core. The overall color is generally redder, indicating an older stellar population with a relatively low star formation rate. There is no indication of strong tidal features or major disturbances. The galaxy appears to be isolated with no interacting companion galaxies.