The galaxy presents as a concentrated, ellipsoidal light distribution with a smooth texture, suggesting a relatively uniform stellar population. The dominant color is a yellowish-orange, indicative of older stars. The galaxy appears to be largely featureless, lacking prominent spiral arms or dust lanes. There is a slightly smaller, less-bright object with a similar color and smooth texture appearing very close to the galaxy's center, which may be a companion galaxy or another concentration of stars within the same galactic halo. There are hints of faint blueish light in the outskirts, potentially indicating some younger star formation but this is not definitive. There appears to be no significant merger activity affecting this object, but there may be a small degree of disturbance to its overall morphology. The galaxy appears to be reasonably isolated. Overall, the morphology suggests a disk system lacking definition due to its distance.
