The galaxy exhibits a generally smooth morphology, suggestive of an elliptical or lenticular type. The central region presents a concentrated luminosity, appearing nearly spherical, with a gradual decrease in intensity toward the outer edges. There is a slight elongation evident, although the overall shape remains relatively round.

The galaxy's color profile appears to be predominantly composed of older stellar populations, displaying a yellowish-red hue. A subtle bluer tint in the central region possibly indicates the presence of a younger stellar population.

There is a hint of minor disturbance or asymmetry within the galaxy’s outer structure, and some faint patches within the galaxy itself may represent star forming regions or dust lanes. The galaxy does not obviously display spiral arm structures.
