The galaxy presents as a smooth, elliptical form. The light distribution appears concentrated toward the center, with a gradual decline in intensity moving outwards. There is a slight elongation, not perfectly spherical but leaning towards an oblate spheroid shape. No distinct spiral arms or other prominent features such as dust lanes are discernible. The color profile suggests an older stellar population, showing yellow-red hues. No signs of ongoing major merging events are immediately apparent. Small irregularities present may indicate minor disturbances or recent smaller interactions.
