The galaxy presents as a disk galaxy, viewed at a moderately high inclination angle. The central bulge appears relatively prominent and smoothly textured, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Extending outwards from the bulge is a fainter, bluer disk, indicating the presence of younger stars and potentially ongoing star formation. There are no apparent spiral arm structures or significant dust lanes visible in this image; it's possible they are too tightly wound or obscured by the inclination. The edges of the disk are poorly defined, with a gradual fading into the background sky. There does not appear to be a substantial, highly active galactic nucleus and there is no strong evidence of any ongoing major merger events.
