The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, relatively featureless morphology. It appears elongated, with a high degree of roundness, though not perfectly spherical. The central bulge is prominent and displays a reddish hue, suggesting an older stellar population. The outer regions transition to a bluer color, possibly indicating the presence of some younger stars or ongoing star formation, although this appears to be minimal. There are no obvious signs of spiral arms or a prominent disk structure. The galaxy does not exhibit any clear indications of a major merger event, though there might be a minor disturbance to the structure, possibly from a smaller interaction. Overall, the galaxy appears to be a fairly evolved system with a dominant smooth component.
