The galaxy presents a generally smooth morphology, appearing largely featureless without readily discernible spiral arms or a distinct bar structure. Its shape is somewhat elliptical, being neither perfectly spherical nor highly elongated. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central regions, indicating a higher concentration of evolved stars. The light appears centrally concentrated, fading gradually towards the outer edges. There is no strong evidence of ongoing major merger activity or tidal disturbances, though subtle asymmetries or minor irregularities in the light distribution may suggest minor past interactions. The object subtends a relatively small angular size, indicative of its considerable distance.
