The galaxy appears as an elliptical or lenticular type, displaying a predominantly smooth morphology. Its shape is more in-between elliptical and a disk shape. There are no readily apparent spiral arms or strong disk features. The galaxy's color profile is somewhat complex. The central region exhibits a more concentrated, yellow-orange hue, likely indicative of an older stellar population and diminished recent star formation. A faint bluer light emanates from regions surrounding the core, which may indicate some ongoing star formation, but not at a significant rate. There are signs of minor gravitational disturbances or possible past interactions with other galaxies. There are no clear indications of a major merger event in progress. The overall appearance suggests a galaxy with a substantial mass and moderate star formation rate.
