The galaxy presents as a relatively compact object with an apparent elliptical morphology. A bright central bulge is prominent, exhibiting a concentrated luminosity profile. There is evidence of a faint, disklike structure extending from the central region. The bulge appears smooth in texture, with an absence of significant dust lanes or distinct star-forming regions. A subtle color gradient is observable, transitioning from a bluer hue in the inner regions to a redder hue in the outer extents of the disk. Minor disturbances are seen in the disk morphology, hinting at potential minor interactions or internal instabilities within the system. The overall appearance suggests a galaxy that is transitioning towards a more passive, early-type morphology, and it is likely at a considerable distance.
