The galaxy presents as a moderately sized, somewhat elliptical structure. It has a smooth, diffuse appearance, with a central region of higher luminosity that gradually fades into the surrounding space. There's a slight elongation, suggesting it might be an elliptical galaxy closer to the "in between" shape. No distinct spiral arms or bars are discernible. The color profile indicates a higher concentration of older stars in the central bulge, with a hint of blue suggesting the presence of some younger stars or ongoing star formation in the outer regions. There is no sign of any ongoing mergers or major disturbances.
