The galaxy presents an elliptical morphology, although not perfectly spherical. It shows a central bulge that transitions into a more diffuse disk. The color gradient indicates an older stellar population concentrated within the galactic center, which appears yellowish. Faint blueish regions are visible within the disk, potentially suggesting some ongoing, but limited, star formation. The overall structure appears relatively undisturbed, with no major signs of ongoing or recent merger activity. There are minor disturbances that are potentially tidal in nature. The galaxy appears to be a relatively massive system, given its size and apparent luminosity.
