The galaxy presents a morphology consistent with a spiral or disk galaxy, though the viewing angle is not edge-on. A central bulge appears prominent, exhibiting a yellowish hue indicative of an older stellar population. Surrounding the bulge, a disk component is visible, displaying a bluer tint, suggesting the presence of younger, hotter stars and ongoing star formation. The spiral arms are not well-defined, but a hint of a spiral structure can be inferred from the uneven distribution of light within the disk. There's an apparent lack of significant dust lanes. No signs of a major merger are apparent. Overall, the galaxy appears to be undergoing moderate star formation activity. The galaxy is of intermediate mass, somewhere around 10 to the 10th power of the mass of the sun.
