The galaxy appears to be a relatively compact, elliptical system. Its light profile exhibits a smooth, centrally concentrated morphology with no obvious spiral arm structures or prominent dust lanes visible at this resolution. The galaxy's color is predominantly yellowish-orange, suggesting an older stellar population and a relatively low rate of ongoing star formation. The overall shape appears nearly circular. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity, though minor perturbations may be present but are difficult to resolve. The object displays a notable red shift, which implies that it is at an intermediate distance.
