The galaxy presents as a roughly elliptical structure with a prominent central bulge exhibiting a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy display a bluer tint, potentially indicating the presence of younger, hotter stars and some ongoing star formation, though minimal. The galaxy appears relatively smooth in structure, lacking any prominent spiral arms or irregular features. The overall shape is somewhat elongated, but not drastically so. There is no obvious indication of any major merger activity or significant tidal disturbances. A small amount of internal dust extinction cannot be ruled out based on the color gradients. The galaxy is of intermediate redshift.
