The galaxy presents a generally smooth morphology, with a high probability of being classified as such. There appears to be no significant disk structure. The galaxy exhibits an intermediate shape between round and elongated, and a very low chance of being cigar shaped. There is no definitive evidence of ongoing major mergers. However, the galaxy may be undergoing or have recently undergone a minor interaction or disturbance. The galaxy appears to have a relatively low star formation rate. The colors show a trend, with bluer magnitudes being brightest, going to redder magnitudes being less bright.
