This galaxy presents as a relatively smooth, elliptical object. Its central region is dominated by a bright, concentrated core, exhibiting a yellow-orange hue suggestive of an older stellar population. The galaxy's light profile gradually decreases from the core outward, with a smooth transition to the less luminous outer regions. There is very little evidence of spiral arm structure or dust lanes within the disk, which are commonly seen in other galaxies. The galaxy appears to be generally isolated with no obvious signs of ongoing major merger events. Faint reddish regions can be observed within the galaxy's extended halo which could indicate sites of star formation. The overall morphology indicates that the galaxy is likely a relatively massive and evolved system, with a moderate amount of ongoing star formation.
