The galaxy presents as an elliptical morphology, appearing largely smooth in structure. The light distribution suggests a spheroidal shape, but with a slight elongation, hinting at a possible classification between E4 and E6 on the Hubble sequence. There is no evidence of spiral arms or a bar. The central region exhibits a strong concentration of light, indicative of a dense stellar population, possibly an older population given the general yellowish-red hue. The outer regions fade gradually, suggesting a decreasing stellar density with increased distance from the galactic center. There does not appear to be significant dust obscuration or prominent star formation regions within the visible light. The overall appearance suggests a relatively quiescent, evolved system. No signs of major interaction or recent merger events are visible.
