The galaxy appears as a single, relatively smooth object with a concentrated central bulge. Its morphology suggests it is likely an elliptical galaxy or a lenticular galaxy with a dominant spheroidal component. The galaxy exhibits a moderate redshift, indicating it is at a significant cosmological distance. Color gradients across the galaxy are subtle, with a slightly yellower hue in the central region compared to the outer parts. This could indicate an older stellar population dominating the core, while the outskirts may have a slightly younger, bluer population. There is no prominent disk structure, spiral arms, or dust lanes visible. A faint hint of tidal disturbance or interaction is possibly present, but further investigation would be necessary to confirm the presence of any ongoing merger activity. The overall luminosity of the galaxy appears high.
