The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The light distribution appears centrally concentrated with a gradual decrease in brightness outward. The core exhibits a yellowish-orange hue, potentially indicative of an older stellar population or dust obscuration. The galaxy appears to have a slight asymmetry, possibly the result of minor disturbances. There is evidence of a very faint, extended halo surrounding the main body of the galaxy. Low levels of ongoing star formation are likely occurring. Overall, the galaxy seems to be in a relatively advanced stage of its evolution.
