The galaxy presents as a lenticular or early-type spiral, with a dominant, relatively smooth bulge and faint, diffuse disk. The bulge exhibits a yellowish-white color, suggesting an older stellar population with fewer hot, young stars. There is little evidence of distinct spiral arms. The disk is subtly bluer than the bulge, indicating the presence of some star formation. The galaxy appears elongated in shape, with an apparent flattening of approximately 2:1. There are hints of minor disturbances in the outer regions of the disk, potentially indicating a past or ongoing interaction with a smaller object. The overall impression is of a galaxy transitioning from a spiral to an elliptical morphology, with a relatively low star formation rate for its mass.
