The galaxy presents as a relatively smooth, elongated structure. The central region exhibits a concentrated yellowish hue, suggestive of an older stellar population. Moving outwards, the color transitions to a greenish halo indicating regions with ongoing star formation, although at a low rate. The overall shape is somewhat irregular with no distinct spiral arm features visible, possibly due to the viewing angle or the galaxy being an elliptical type. There might be some minor distortions in the morphology, suggesting a potential interaction or past merger event, but it mostly appears undisturbed.
