The galaxy presents as a generally elliptical morphology, with a high degree of central concentration of light. The central region is bright and appears yellowish, suggesting an older stellar population. Moving outward from the center, the light intensity diminishes, and a faint, bluish halo is visible. The overall structure appears relatively smooth, with no obvious signs of spiral arms or major distortions. There might be some minor tidal disturbances. The galaxy appears to be transitioning to a more spheroid shape; the shape seems to be in between round and cigar shaped. The light from the galaxy indicates ongoing, but relatively low, levels of star formation. The color gradients suggest a radial variation in stellar populations, with older, redder stars dominating the core and younger, bluer stars contributing to the fainter outskirts.
