The galaxy presents a centrally concentrated luminosity profile, indicating a significant bulge component. Its overall shape appears elliptical, with a moderate degree of roundness. The galaxy's color profile suggests an older stellar population, with a redder hue dominating the outer regions. There are no prominent spiral arms or significant dust lanes visible. Subtle irregularities in the outer regions suggest possible past or ongoing minor interactions. The overall morphology leans toward a smooth, relatively undisturbed structure. The redshift indicates that the light from this galaxy has been stretched, allowing for a calculation of its distance from us.