The galaxy presents as a roughly elliptical structure, though there is some irregularity to its overall shape. A bright, concentrated central bulge is evident, suggesting the presence of a supermassive black hole and a dense population of stars in the galactic nucleus.

The outer regions of the galaxy exhibit a faint, diffuse glow. This halo appears somewhat disturbed, indicating possible past interactions with smaller galaxies or tidal effects from larger nearby galaxies. The disk is either not very pronounced, or is obscured by dust. There is a faint hint of disturbance in the halo with some irregular extensions, this could indicate minor merging activity, or possibly be an artifact of the image.

The color profile shows a concentration of bluer light in the galactic center and inner regions, potentially indicating ongoing star formation or a younger stellar population. The colors of the outer regions are redder suggesting an older population of stars.
