The galaxy exhibits an elliptical morphology, appearing largely smooth and featureless. The light distribution suggests a high degree of central concentration, with a gradual decrease in intensity outward from the core. The galaxy's color appears yellowish-orange, possibly indicative of an older stellar population and a relative lack of ongoing star formation. There is no clear evidence of spiral arms, a prominent disk, or significant dust lanes. There is also no obvious sign of any major mergers or tidal disruptions. The overall structure suggests a relatively evolved system.
