The galaxy presents as an elongated, elliptical structure. It exhibits a generally smooth appearance, with a concentrated central region or bulge. There is a distinct blueish hue emanating from the main body of the galaxy, which suggests a component of younger stellar populations. The overall shape could be described as a flattened spheroid, with a significant fraction leaning towards an in-between roundness. No prominent spiral arms or disk-like features are immediately apparent. There is a very slight indication of some minor disturbance or irregularity, though it seems to be relatively settled, and not in the throes of any major merger activity.
