The galaxy appears as a singular, relatively smooth object with a concentrated central bulge. The overall shape seems generally round, though there is a slight elongation, possibly indicating it is an elliptical galaxy. The color distribution reveals a central yellowish-golden hue that gradually fades outward to a more teal color. There is no obvious spiral arm structure or any indications of major disturbances such as tidal tails or multiple nuclei. No presence of dust lanes is discernible. Based on the color, this galaxy appears to be composed of an older stellar population. There may be very faint disturbances suggesting a minor gravitational interaction, although they could also be image artifacts.
