The galaxy appears as a single, relatively smooth object with a concentrated central bulge. It exhibits a generally elliptical shape, tending towards roundness. The color profile indicates an older stellar population, leaning towards redder hues, with a subtle gradient towards bluer tones at the periphery. There's no discernible evidence of spiral arms or a distinct disk structure. No major disturbances are observed within the galactic structure, indicating it is likely not undergoing a major merging event.
