The galaxy presents as a concentrated, moderately luminous object with a generally smooth appearance. Its color profile suggests a dominant population of older stars, emitting primarily in the redder wavelengths. There is a slight elongation to the galaxy's form, though it appears mostly rounded. No significant tidal features or signs of recent major mergers are apparent. Faint irregular and clumpy edges are visible, indicating some active star formation. The galaxy is not perfectly spherical, with a mild deviation towards a more flattened ellipsoidal shape.
