The galaxy exhibits a generally smooth morphology, appearing as an elliptical or lenticular type galaxy. The central region presents a concentrated, bright, yellowish core. Fainter, blue-ish light emanates from the surrounding disc. The galaxy is observed to be elongated, with its shape categorized as leaning towards in-between round and cigar shaped. There appear to be no significant signs of major disturbances from a recent merger, although there might be minor disturbances present. Based on the color and the concentration of light in the core, we can expect the galaxy to host stars that are generally older. I would categorize this galaxy as being a relatively massive system with moderate star formation activity.