The galaxy presents a generally smooth morphology, with a discernible elliptical shape. Its color profile indicates a concentration of older stellar populations, particularly in the central bulge, which exhibits a yellowish hue. The outer regions show hints of bluer colors, suggesting ongoing, albeit modest, star formation activity. There is a slight visual asymmetry to the galaxy, possibly indicative of a minor gravitational disturbance or past interaction with another galaxy, or could simply be an artifact of the viewing angle. There are no well-defined spiral arms or bar structures visible; the light distribution appears relatively uniform and the galaxy is largely featureless overall. The size is appreciable; it is not a dwarf galaxy. Based on the available data it can be reasonably inferred the galaxy is an early-type spiral, or perhaps elliptical galaxy.
