The galaxy appears as a moderately luminous, isolated object, exhibiting a smooth, elliptical morphology. The light distribution suggests a generally well-mixed stellar population with minimal discernible substructure. The galaxy's shape is elongated, leaning towards a cigar shape, but predominantly classified as "in-between" a perfect circle. There may be signs of minor tidal disturbance or past interactions, but the dominant visual impression is one of an undisturbed system. The colors observed indicate a relatively evolved stellar population, consistent with a low ongoing star formation rate. The object is relatively compact, indicating a moderately sized system. There isn't any evidence of active galactic nuclei activity or a very high rate of star formation.
