The galaxy exhibits a generally smooth morphology with a slightly elliptical shape. The light profile appears more centrally concentrated, indicating a relatively old stellar population with minimal ongoing star formation. The central region displays a bluish hue, possibly suggesting the presence of a central active galactic nucleus or a compact region of recently formed, hot stars. However, the blue color may also be artificially caused by a high redshift or high levels of dust attenuation, which is not clear here. The surrounding outer regions show hints of a faint, diffuse halo. There is a very small likelihood that there could be faint disturbances present, suggestive of past minor interactions, or an ongoing merger.
