The galaxy appears as a generally smooth, elliptical structure. It is relatively compact, with an estimated effective radius around 4.4 kpc. The galaxy exhibits a high degree of circular symmetry, presenting a rounded morphology. There is no apparent evidence of major mergers or significant tidal disturbances. The light distribution suggests an evolved stellar population, consistent with a relatively low star formation rate. The galaxy displays a redder color, hinting at a population of older stars and a lower concentration of young, blue stars and gas. Overall, the galaxy appears to be a quiescent elliptical galaxy with a substantial mass, at a redshift of approximately 0.27.
