The galaxy presents as a single, dominant structure, likely an elliptical or lenticular galaxy due to its smooth, largely featureless morphology. Its shape appears somewhat rounded, with a slight elongation giving it an overall elliptical form. The color gradient observed transitions from a predominantly reddish-orange core to a greenish hue in the outer regions. This color variation suggests potential differences in stellar populations or dust content across the galaxy's structure, with the core possibly dominated by older, redder stars and the outer regions showing some evidence of younger, bluer stars or more active star formation, or the prevalence of ionized gas emission. There is no clear evidence of spiral arms or a distinct disk component. No significant signs of ongoing or recent major mergers are visible, but a very slight asymmetry might hint at a minor interaction in its past or current state. The galaxy's size appears relatively compact, suggesting a smaller physical extent.
