The galaxy presents as a spiral type, observed at a significant inclination angle relative to our line of sight. The disk structure is evident, showing a relatively bright and extended nature. Spiral arms are apparent, though not sharply defined. The central bulge appears moderately prominent and concentrated, contributing significantly to the overall luminosity of the galaxy. A strong bar feature is visible spanning across the central region of the galaxy, oriented roughly along the apparent major axis. No major merging events are readily discernible, although some minor irregularities within the disk may indicate past interactions. Overall, the galaxy exhibits a morphology consistent with a barred spiral galaxy, characterized by a moderate-sized bulge, prominent bar structure, and a relatively well-defined disk with observable spiral arms.
