The galaxy presents as a relatively compact object with a somewhat elliptical morphology. A bright central core dominates the luminosity profile, suggesting the possible presence of an active galactic nucleus or a high concentration of stars in the galactic bulge. There appears to be a faint disk component surrounding the central core, although it is not well-defined. Some minor irregularities are present in the outer regions of the disk. These may be due to tidal interactions. The overall color of the galaxy appears to be somewhat blueish. This would indicate a potentially significant population of young, hot stars and ongoing star formation processes, particularly in the faint disk. There are also some hints of redder color towards the central core. This could indicate an older stellar population or dust obscuration. A careful investigation into the color gradients and spectral features is needed.
