The galaxy appears as a moderately bright, somewhat elongated object with a smooth, diffuse morphology. The central region exhibits a concentrated, yellowish-orange hue, indicating a population of older stars. Fainter, greenish-blue tendrils extend outwards from the core, potentially indicative of regions of ongoing, albeit subdued, star formation. There is no strong evidence of spiral arms or a well-defined disk. Minor disturbances are possible, but the overall structure is relatively undisturbed, suggesting a lack of recent major mergers. The galaxy has a moderate physical size.
