The galaxy appears to be a relatively smooth, elliptical or lenticular type system. Its overall shape is elongated, presenting a cigar-like or prolate morphology. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population likely composed of Population II stars. There is a lack of prominent spiral arms or dust lanes visible. The galaxy does not display strong signs of ongoing major merger activity or significant tidal disturbances, although a possible minor interaction with a smaller object located nearby cannot be ruled out. The color gradient from the central bulge to the outer regions is subtle, with a slight decrease in the yellowish hue, potentially indicating a younger stellar population in the outer regions, although this is not highly pronounced.
