The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish-orange hue, indicating an older stellar population with minimal ongoing star formation. The galaxy displays an elongated shape, leaning towards an in-between roundness, showing some ellipticity. There is no discernible evidence of major mergers or significant tidal disturbances affecting its morphology, suggesting it is a relatively isolated and evolved system. While a faint disk-like structure might be present, it is not particularly prominent. The galaxy's colors suggest that it is composed mostly of evolved stars, and is therefore an older, redder system.