The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. The core is a bright, yellowish-white, suggesting a population of older stars. There is a gradual decline in luminosity from the core outwards, with the outer regions displaying a bluer hue, perhaps indicating the presence of a younger stellar population, although at a significantly lower rate. The overall shape approximates a flattened spheroid, with a slight elongation visible. There is no discernible spiral arm structure or dust lane present. Faint tidal features are not obviously seen, the galaxy seems to be isolated with no major gravitational disturbance.
