The galaxy presents as a spiral, although its disk appears somewhat disturbed. Its orientation is oblique to our line of sight. A prominent central bulge dominates its appearance, with indications of spiral arms extending from this central region, although their structure is not well-defined and appears flocculent. The bulge exhibits a yellowish hue, suggesting an older stellar population, while the disk shows patches of blue, hinting at regions of active star formation. The overall color is intermediate between red and blue, indicating a mix of stellar populations. The isophotes exhibit a moderate ellipticity, suggesting some flattening of the galaxy. There is an indication of a bar feature in the galaxy's central region. Faint tidal features are visible. Overall, the galaxy appears to be undergoing a minor merger or interaction event, which has contributed to the disturbance in its spiral structure.
