The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its shape is somewhere between round and elongated. There is no evidence of significant tidal disturbances or recent major mergers. The color gradient suggests an older stellar population dominates, especially in the central bulge, transitioning to slightly bluer hues in the outer regions. The lack of prominent spiral arms or dust lanes is consistent with an elliptical or lenticular classification. Based on the observed characteristics, it seems to be a galaxy with a relatively low star formation rate.
