The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. The galaxy exhibits a color gradient, transitioning from a yellowish core to a fainter, bluer halo. There may be minor visual signs of disturbance in the outer regions, but these are subtle. The shape is somewhat elongated, appearing more "in between" than perfectly round or cigar-shaped. The light distribution suggests the presence of an older stellar population dominating the central regions, while the outer regions may host younger, bluer stars and a low amount of star formation. Overall, the galaxy appears to be relatively isolated, without any significant signs of interaction or merging.
