The galaxy appears as a lenticular or early-type spiral with a relatively smooth texture. It presents with a prominent central bulge, which is elongated and displays a gradual decrease in luminosity from its core. There's a faint hint of a disk structure surrounding the bulge, but it lacks well-defined spiral arms. The color profile suggests a population of older stars, indicating low rates of current star formation. There are minor signs of tidal disturbance, though no significant merging event appears to be taking place currently. 