The galaxy presents as an elliptical-like system with a high degree of central concentration. The core region exhibits a bright, yellowish hue, suggesting an older stellar population dominating the central area. Moving outward from the core, the galaxy gradually fades in intensity. The overall structure appears relatively smooth, with little evidence of significant spiral arm structures or prominent dust lanes. There's a slight bluing in the outer regions indicating some younger stars. The galaxy's shape is roughly circular or slightly elliptical, with no obvious signs of major tidal disturbances or ongoing mergers. The overall appearance suggests a galaxy that is undergoing relatively low levels of star formation.
