This galaxy exhibits a spiral morphology. The disk is not viewed perfectly face-on, presenting a slightly inclined profile. Prominent spiral arms emanate from a central bulge region. These arms are well-defined and display a somewhat open winding pattern. Evidence suggests a bar structure bisecting the central bulge. The bulge appears moderately sized relative to the overall galactic disk. While the overall structure is largely intact, indications of a possible minor disturbance are present, potentially hinting at a past or ongoing interaction.
