The galaxy appears as a centrally concentrated object with an overall smooth morphology. It exhibits a moderately elliptical shape, with the ratio of the major to minor axis being approximately 5:1, meaning it is somewhat cigar-shaped. The light distribution seems to be fairly uniform across the galaxy, lacking any prominent spiral arm structures or distinct features typically associated with ongoing major mergers. There may be some minor disturbances, as the galaxy appears slightly asymmetrical on closer inspection, but the overall structure suggests it is not currently undergoing significant interaction with another galaxy. Its color index suggests a population of evolved stars.
