The galaxy presents a generally smooth and elliptical morphology. The light distribution appears centrally concentrated, gradually fading outwards from the core. The galaxy's shape is not perfectly circular, showing a slight elongation suggestive of an intermediate ellipticity. The color profile exhibits a predominantly yellowish-red hue, indicative of an older stellar population with fewer young, hot stars. There are faint traces of blue light visible at the edges of the object, perhaps indicating some localized star formation. No prominent spiral arms or dust lanes are discernible. There are some subtle irregularities to its edge, which may indicate minor interactions or disturbances.
