The galaxy presents as a spiral galaxy with a discernible disk structure oriented at a relatively high inclination with respect to our line of sight. The central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a significant population of older stars. Faint, loosely wound spiral arms extend from the bulge, displaying regions of lower surface brightness and a mottled texture indicative of star-forming regions within the disk. The dust lanes appear subtle, tracing the inner edges of the spiral arms and contributing to the patchy appearance. Overall, the galaxy exhibits a regular morphology, and there is no visually apparent evidence of a major ongoing merger, though minor disturbances can not be ruled out. The disk demonstrates a flattened shape with a slight ellipticity.
