The galaxy appears to be an elliptical or lenticular galaxy, viewed at an oblique angle. It exhibits a smooth, diffuse morphology with no distinct spiral arms or prominent dust lanes visible. The central bulge is moderately prominent, showing a gradual transition to the outer regions of the galaxy. The color gradient suggests a stellar population that is generally older, with bluer regions potentially indicating areas of recent, albeit low level, star formation. The overall shape approximates a flattened spheroid, with some elongation possibly giving it a cigar-like appearance. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity.
