The galaxy presents as a diffuse, centrally concentrated object with a generally smooth appearance. Its overall shape is elliptical, exhibiting a high degree of roundness. There is a notable lack of distinct spiral arm structures. Color gradients suggest a population of older stars dominating the light output, implying a relatively low rate of ongoing star formation. Faint disturbances visible may indicate a prior interaction with another galaxy, possibly a minor merger event, though the current morphology is not severely disrupted. The galaxy appears relatively isolated.
