The galaxy presents a largely smooth appearance with a slight elongation, suggesting a possible elliptical morphology, though a disk component cannot be entirely ruled out. There are no prominent spiral arms or distinct features that would clearly indicate a spiral structure. The central region displays a higher concentration of light, indicative of a bulge or core. The galaxy appears to be a relatively quiescent system, exhibiting low star formation activity. There is no obvious sign of a major merger event, though subtle irregularities in its shape could indicate a minor interaction or disturbance in the past. The overall color of the galaxy suggests a population of older stars, consistent with its low star formation rate. The galaxy's light is redshifted, indicating it is at a considerable distance from us, expanding along with the universe.
