The galaxy appears as a predominantly smooth, elliptical-shaped structure with a concentrated central bulge. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the core region, which fades to a slightly bluer tint moving outwards from the galaxy center. There is little evidence of spiral arms or significant dust lanes. The galaxy's morphology indicates it's likely a relatively evolved system, possibly a lenticular or elliptical galaxy, with a quiescent star formation rate. No signs of tidal disturbances or ongoing merger activity are apparent.
