The galaxy presents as a luminous, relatively smooth object with an overall elliptical morphology. The core exhibits a concentrated, bright region, suggesting a significant stellar population density. The overall color appears yellowish-orange, indicating an older stellar population with fewer young, hot stars. There is a possible faint disk structure. The isophotes appear mostly regular, with some minor distortions possibly indicating a past or ongoing interaction or minor disturbance. No prominent spiral arms are discernible. Based on the observed characteristics, this galaxy is likely a massive elliptical or lenticular galaxy at a considerable distance.