The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The light distribution indicates a lack of prominent spiral arms or a distinct disk structure. Its color appears to be somewhat redder, suggesting an older stellar population and/or a considerable amount of dust obscuration. There is no apparent ongoing major merger activity or significant tidal disturbances; however, there may be very minor distortions. The galaxy's shape appears to be moderately rounded, not highly elongated or cigar-shaped.
