The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a high concentration of light, appearing bright yellow in this color representation, likely indicating an older stellar population. Moving outwards from the core, the light gradually fades into a dimmer, more diffuse halo. A slight asymmetry is observed in the outer regions, with an extension towards the lower part of the image showing a hint of green, suggesting a region of relatively more recent, though limited, star formation. Overall the galaxy appears to be a relatively massive system exhibiting a relatively low star-formation rate. There appears to be evidence of some interaction with other galaxies.
