The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. There is little discernible structure such as spiral arms or a prominent bar. The galaxy exhibits a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. The color profile suggests a population of older stars, with a slightly redder hue overall. There is no clear evidence of a major ongoing merger or tidal disturbance, although subtle asymmetry or minor disturbances cannot be ruled out based on the image alone. The galaxy's core region shows a somewhat brighter concentration of light, which may indicate the presence of a central bulge. While the galaxy appears relatively isolated, deeper observations would be required to exclude the presence of faint companions or tidal streams.
