The galaxy presents a moderately luminous profile. It exhibits an elongated, somewhat cigar-shaped morphology. The light distribution appears relatively smooth, lacking distinct spiral arm structures. The color gradient suggests a population dominated by older stars, as indicated by the reddish-yellow hue. There may be some evidence of minor disturbances or interactions in the form of slightly irregular light distribution. The overall structure suggests a system in the transition from a spiral to an elliptical galaxy or possibly a lenticular galaxy. No strong evidence of ongoing major star formation activity is apparent. The galaxy is estimated to be a considerable size.
