The galaxy appears as a somewhat elongated, flattened structure, indicative of a possible disk galaxy viewed at an angle. The central bulge region is bright and concentrated, exhibiting a yellowish hue, suggesting a population of older stars. The overall color of the galaxy trends toward redder hues, particularly in the central regions, implying a relatively low rate of recent star formation. The disk component, while present, does not show distinct spiral arm structures. There is a hint of some irregularities or faint disturbances in the disk, possibly indicating past interactions or minor merging events. Based on the galaxy's shape, it leans toward a cigar shape more than a perfect circle. Most likely it is not undergoing any significant merging events. The galaxy is relatively smooth in appearance overall with some features. 
