The galaxy appears to be a relatively smooth, elliptical-like object at a considerable distance. Its core exhibits a yellowish-orange hue, suggesting a population of older stars. Moving outward from the core, the color transitions to a more greenish tint, possibly indicating a younger stellar population or regions of ongoing star formation. There appears to be minimal dust or distinct structural features such as spiral arms or a prominent bar. The overall morphology suggests a well-mixed and relaxed system, possibly resulting from the merging of smaller galaxies in its past. The galaxy's shape appears mostly round, lacking significant elongation or asymmetry. There is no evidence of ongoing major mergers, tidal tails, or significant disturbances in the surrounding area. It is a fairly isolated system, although its faintness makes a full characterization difficult.
