The galaxy presents as a cigar-shaped morphology. It exhibits a smooth, elongated central bulge which appears yellowish-white, suggesting an older stellar population. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly bluer than the central bulge; this may indicate more recent star formation activity. There is no apparent spiral arm structure or significant dust lane obscuration, suggesting the structure is likely of an elliptical type. The galaxy appears relatively undisturbed, without any visible signs of major merging events.
