The galaxy exhibits an elliptical morphology, elongated in shape, and with a relatively high Sersic index, suggesting a prominent bulge. The central region displays a concentrated luminosity, indicating a high stellar density.  Color gradients are visible, with the core appearing more yellowish, possibly indicating an older stellar population, while the outer regions exhibit a bluer hue, suggesting the presence of younger, hotter stars. A faint, disturbed feature appears in the northern part of the galaxy; this may be a tidal tail resulting from a past interaction with another galaxy. Overall the galaxy appears to have a relatively low rate of star formation, consistent with a more evolved system.
