The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. Its color profile suggests an older stellar population, with a yellowish hue dominating the core region. The light appears to gradually fade from a bright central bulge outward, showing a very slight flattening. There is no clear evidence of spiral arms or prominent dust lanes. The lack of distinct features points towards a galaxy that is relatively undisturbed. The limited color variation implies a low star formation rate within the observed timeframe.
