The galaxy presents as a somewhat smooth, lenticular-like structure. Its color appears primarily yellowish-orange, possibly indicative of an older stellar population and lower ongoing star formation. The central bulge seems prominent, exhibiting a slightly higher concentration of light compared to the outer regions. The edges of the galaxy appear diffuse, lacking sharp boundaries, suggesting a gradual decrease in stellar density with increasing radius. There may be some subtle indications of a possible minor disturbance, such as a slight asymmetry or warp in the overall shape, but the galaxy otherwise shows a relatively undisturbed morphology. There is no apparent disk component.
