The galaxy appears to be an elliptical type, characterized by a smooth, diffuse light distribution. There's a pronounced central bulge that graduates in luminosity from a bright yellow-orange core to a softer, more diffuse light. This suggests an older stellar population concentrated at the core. Extending outward from the core is a fainter, blueish halo or disk structure. The overall form is consistent with a galaxy that may have recently undergone a minor merger event, or possibly exhibiting some faint tidal features that could be indicative of gravitational interactions. There is not a strong presence of concentrated dust lanes.
