The galaxy presents as a spiral type, with two prominent, loosely wound spiral arms emanating from a central bulge. The arms exhibit a mottled texture, suggesting regions of active star formation, with a subtle bluish tint indicative of the presence of young, hot stars. The central bulge appears relatively smooth and concentrated, displaying a yellowish-white hue, potentially indicating an older stellar population. A faint bar structure appears to transect the central bulge, but is not very well defined. The disk is inclined slightly, but not perfectly edge on. Faint dust lanes may be present within the spiral arms, though the image resolution makes it difficult to ascertain conclusively. The overall morphology suggests a galaxy in a relatively late stage of its evolutionary sequence, showing established spiral structure and ongoing star formation. There are also some signs of tidal disturbance.
