The galaxy presents as a spiral type, although with a somewhat blurred morphology possibly due to distance or image quality. The central bulge is a prominent, elongated feature exhibiting a yellowish hue, suggesting an older stellar population within the core. A distinct bar structure appears to bisect the bulge along its major axis. Two tightly wound spiral arms emanate from the ends of the bar. The spiral arms are traced by bluer regions, indicative of ongoing star formation and a younger stellar population. The galaxy's disk appears to have a slight tilt relative to our line of sight, as evidenced by its elliptical shape. No major signs of disturbance or merging activity are visually apparent, although some minor irregularities in the spiral arm structure suggest possible gravitational interactions or internal dynamics. The size of the bulge is relatively moderate in comparison to the overall disk size.
