The galaxy presents as a singular, centrally concentrated object with a generally smooth morphology. The light is fairly symmetrical, displaying a gradual decrease in intensity outward from a bright, unresolved core. The galaxy appears relatively round in shape. There are no prominent spiral arms, bar structures, or obvious signs of recent major merger activity discernible in the image. The color appears mostly uniform, with a slightly yellowish hue throughout. The light distribution suggests a galaxy dominated by an older stellar population. There might be very faint indications of a diffuse, extended halo surrounding the central region, but the low resolution makes definitive assessment difficult.
