The galaxy presents a generally smooth and rounded morphology. There is a noticeable central bulge that dominates the overall light profile. Faint, diffuse extensions surround the central region, indicating a possible halo or outer disk. There is little evidence of spiral arms or significant dust lanes, though the resolution is limited. The color appears relatively uniform, with a slight reddish hue suggesting a population of older stars. Based on the size and luminosity, this is likely a massive galaxy exhibiting a moderate rate of star formation. There is no clear indication of any major ongoing merger events, although some minor disturbance in the outer regions cannot be ruled out based on the image alone.
