The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, with a radial decrease in luminosity outward. The galaxy displays a slightly elongated shape, but is generally quite round. There is a faint hint of a disk structure, although it is not very pronounced. The color profile suggests an older stellar population, with a redder hue overall, with a possible region of recent star formation. There is no apparent interaction with any nearby galaxies, but there is a faint disturbance in the morphology which could suggest a minor interaction.
