The galaxy presents as a somewhat elongated, luminous structure. A bright, concentrated central bulge appears yellowish, indicating a dominant population of older stars. Extending outwards is a faint disk structure oriented at a significant angle to our line of sight. The disk appears to be somewhat diffuse, with little to no discernible spiral arm structure within the resolution of the image. A slight bluer hue may be present within the disk regions, hinting at ongoing, although likely limited, star formation. The overall morphology suggests a galaxy that is transitioning from a more active, star-forming state to a relatively quiescent one. There may be some gravitational interaction or minor disturbance occurring, given the slightly asymmetric outer edges of the galaxy.
