The galaxy presents as a relatively compact system with a dominant central bulge. There is some indication of a faint, diffuse disk component extending outwards, but distinct spiral arms are not readily apparent. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the disk show hints of bluer light, potentially indicating areas of more recent star formation, although the details are indistinct. Overall, the galaxy appears to possess a moderate mass and may be undergoing relatively low levels of star formation. There is a possible companion galaxy or tidal feature that shows a yellow-orange light.
