The galaxy appears as a moderately inclined disk galaxy. The central bulge is prominent and diffuse, with a relatively high surface brightness compared to the disk. There appears to be a degree of patchiness or granularity within the disk, suggesting some level of resolved structure possibly due to the presence of stellar populations or dust clouds. The overall color of the galaxy is a bluish-white, hinting at a substantial presence of younger, hotter stars contributing to the overall light output. The shape appears relatively smooth and undisturbed, with no obvious signs of major mergers or tidal disruptions. There are faint blueish regions along the disk, perhaps indicative of star forming regions. The galaxy possesses a moderate angular size.
