The galaxy appears to be a spiral galaxy seen at an oblique angle. The spiral arms are not clearly defined, with evidence of some disruption or flocculence. The galaxy exhibits a generally smooth and centrally concentrated bulge. There is some color variation across the galaxy, with bluer regions potentially indicating areas of more recent star formation within the spiral arms and a redder hue toward the bulge, possibly indicative of an older stellar population. There is no obvious presence of a strong central bar feature. A faint tidal tail is visible, indicating the potential for some sort of past merging event. Overall the galaxy seems to be undergoing some sort of interaction that is disrupting its features.