The galaxy presents as a centrally concentrated, luminous object, with a roughly elliptical morphology. Its structure is generally smooth in appearance, suggesting an older stellar population and potentially a relatively quiescent evolutionary state. There is a subtle elongation. The color profile indicates a redder hue, indicative of older stars or dust obscuration, but with a significant amount of blue wavelengths suggesting star formation is still occurring. There is no distinct evidence of spiral arms or a prominent disk structure. Evidence suggests a weak rate of star formation. There may be only slight morphological disturbance.
