The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology suggests an elliptical galaxy, exhibiting a high degree of symmetry. The color profile indicates a dominant population of older stars, with the galaxy appearing more luminous in the redder bands. The galaxy has a slightly elongated shape, but is mostly round. There is no obvious evidence of significant ongoing star formation or prominent spiral arms. The galaxy does not appear to be undergoing any major merging activity. The absence of distinct features suggests a quiescent evolutionary state.
