The galaxy presents as a largely elliptical morphology with a smooth light distribution, indicating a lack of prominent spiral arms or distinct features. The color profile appears to be generally redder, particularly in the central regions, which suggests an older stellar population and reduced on-going star formation. There is a slight elongation, but it is generally quite round. There is no obvious evidence of an active galactic nucleus or ongoing merging activity, though a minor disturbance cannot be completely ruled out at this resolution. Based on the color and morphology, this galaxy appears to be an evolved system.
