The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth morphology. The galaxy appears to be largely featureless. A slight elongation is observed along its major axis, with a small deviation from perfect circularity. The central region displays a higher concentration of light, indicative of a galactic nucleus. The galaxy exhibits a color gradient, transitioning from a yellower core to bluer hues in the outer regions. This suggests the possibility of ongoing star formation or a more complex stellar population distribution within the galaxy. The galaxy shows no signs of major merging activity or significant tidal disturbances.