The galaxy exhibits a generally smooth morphology, suggestive of an elliptical or lenticular type. It appears roughly circular in shape, with only slight deviations from perfect roundness. There is a bright central bulge that dominates the overall luminosity profile, indicating a high concentration of stars in the galactic nucleus. The radial color gradient suggests that the central region is redder than the outer regions. This could be due to the presence of older stellar populations in the center, or dust obscuration. Faint features are present in the outer regions, hinting at the possibility of a diffuse disk component or tidal interactions, but they are not prominent. There is no obvious evidence of spiral arms or strong dust lanes. The overall color is slightly blue, suggesting some on-going star formation, but is is more likely that the color is being contributed from old main sequence turnoff stars. The image reveals no apparent signs of a major merger, or any tidal tails, suggesting that the galaxy has likely not undergone major interactions recently.
