The galaxy presents as a relatively smooth, elliptical-like structure. The core is quite bright, exhibiting a concentrated luminosity indicative of a significant stellar population and possibly an active galactic nucleus. The overall color appears yellowish-white, suggesting an older stellar population with a lower rate of ongoing star formation. There is very little, if any, evidence of spiral arms or a distinct disk structure. The galaxy exhibits a gradual decline in luminosity from its core to its outer regions. There do not appear to be any major disturbances or tidal features suggesting a recent major merger. However, there are a few indications of minor disturbances in the outer regions. The galaxy appears primarily undisturbed and well-established.
