The galaxy presents as a somewhat elongated, cigar-shaped structure. The central region displays a higher surface brightness, appearing as a concentrated, yellowish-white core. Moving outwards from the core, the light gradually diffuses into a fainter, bluer halo. There's a slight indication of a disk-like structure, but no distinct spiral arms or prominent features are discernible. The galaxy appears relatively smooth overall with a hint of disturbance in the outer regions, possibly indicative of minor gravitational interaction or past merger events. The colors suggest a population of older stars in the core, with ongoing or recent star formation in the outer regions contributing to the blue hue.
