The galaxy appears to be an elliptical or lenticular type, with a largely smooth and featureless morphology. It is characterized by a central bulge and a generally spheroid shape. The light distribution is concentrated towards the center, exhibiting a radial gradient with decreasing intensity outward. The galaxy has a slightly elongated shape, possibly indicating some degree of rotational flattening. The overall color suggests an older stellar population, though the presence of some blue light indicates that there may still be some ongoing star formation within it. The galaxy does not appear to be undergoing any major merger events, though there appears to be a faint tidal stream that suggest a minor merger or interaction in the past. The galaxy has a estimated mass of around 10^10 solar masses and a low specific star formation rate.
