The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests an elliptical or lenticular type. The light distribution appears nearly uniform, with a noticeable radial concentration towards the nucleus. The galaxy has an overall slightly elongated shape, but it is not highly flattened. There's some hint of a disk structure, although it is not very prominent. There does not appear to be evidence of significant ongoing merger activity or major disturbances in its structure, although there are some minor signs of disturbances. The color profile suggests the presence of a somewhat older stellar population with ongoing star formation. The object is approximately 5 kiloparsecs in radius and has a stellar mass on the order of 10^10.5 solar masses. The specific star formation rate is also slow, indicating that the rate of new star formation is low compared to the total stellar mass of the galaxy.
