The galaxy presents as a moderately sized spiral galaxy with a prominent central bulge. The bulge appears yellow-white, suggesting an older stellar population. Faint and somewhat diffuse spiral arms are visible, indicating an ongoing, albeit potentially subdued, star formation activity. There is evidence of a bar structure, with the galaxy likely possessing a weak bar. The galaxy appears to have an interaction or possible merger with a smaller object, implying a merger event in the past. There seems to be an equal chance of merger events or disturbances.