The galaxy presents as a relatively small spiral galaxy, viewed at a near edge-on inclination. A distinct central bulge is visible, exhibiting a smoother, more concentrated light profile. Fainter spiral arms extend outward from the bulge, with some clumpy features of slightly brighter regions of presumed star formation. The galaxy appears moderately blue, suggesting a population of young, hot stars. While generally appearing symmetrical, there may be minor distortions or a faint tidal tail on one end, potentially indicative of past or ongoing gravitational interactions.
