The galaxy presents a generally smooth, elliptical morphology. The core appears bright and concentrated, with a color profile leaning towards the redder end of the spectrum. The overall structure lacks prominent spiral arms or distinct features, suggesting an evolved system, possibly with a significant population of older stars and a relatively low rate of star formation. There is some evidence of minor disturbances or potential merging activity in its morphology, though the primary shape remains relatively undisturbed. The galaxy shows an approximate physical diameter of 7.65 kpc.
