The galaxy presents a largely smooth and rounded morphology. The central region displays a concentrated luminosity gradient, appearing bright and yellowish, suggesting an older stellar population likely dominating the core. This core is surrounded by a fainter, more diffuse halo. Faint blue tinges are visible at the edges, hinting at the presence of younger, hotter stars and potentially ongoing star formation. There is no visible structure indicative of spiral arms or a prominent disk component. No obvious signs of tidal disturbances or major mergers are discernible. The galaxy appears to be relatively undisturbed.
