The galaxy presents as a moderately luminous object with an elliptical morphology. It exhibits a central bulge that is noticeably brighter and more concentrated than the surrounding disk. The bulge displays a yellowish-orange hue, suggesting an older stellar population. The disk is less defined, appearing somewhat smoother with a subtle blue tinge. The galaxy's overall shape indicates a slight elongation, with the ratio of its major to minor axis approximately 2:1. There is no discernible evidence of strong spiral arm structure or significant dust lanes. The galaxy does not appear to be undergoing any major merger events or tidal interactions. There might be some minor disturbances in the outer regions of the galaxy. Overall, it appears to be a relatively evolved galaxy with a moderate rate of star formation.
