The galaxy presents as a relatively smooth, disk-shaped structure with a prominent central bulge. The color gradient suggests an older stellar population, particularly within the bulge region which appears yellowish-orange. The disk, viewed at a significant inclination, exhibits a subtle bluer hue at the edges, possibly indicating ongoing star formation. The overall shape is elongated, with the major axis being considerably longer than the minor axis. No distinct spiral arms or bar structures are discernible in this image. There is no evidence of any major mergers or tidal disturbances. Faint light extends outwards from the central region, fading gradually into the background.
