The galaxy presents as a concentrated, elliptical-like object with a smooth morphology. The light profile appears centrally concentrated with a gradual falloff in intensity towards the outer edges. The galaxy's core exhibits a yellowish-white hue, suggesting the presence of an older stellar population. No distinct spiral arm structures or prominent dust lanes are discernible. There is little evidence of ongoing major merging events, but the presence of a very minor disturbance cannot be completely ruled out. Overall, the galaxy exhibits a smooth, rounded shape, with a relatively high degree of symmetry.
