The galaxy presents a generally smooth morphology, although subtle features are discernible. Its overall color is predominantly yellow-orange, suggesting an older stellar population with a significant presence of evolved stars. A central, brighter region implies a concentration of stellar density towards the core. The galaxy exhibits a slight elongation. There might be a faint indication of minor disturbances in the outer regions, possibly indicative of past or ongoing interaction, but it appears mostly undisturbed. There is no clear sign of spiral arms.