The galaxy presents as a generally smooth object, elliptical in shape, with a concentrated central bulge. The light profile is centrally concentrated, decreasing in intensity with radial distance. Some subtle color variations are noticeable. The central region exhibits a yellowish hue, suggesting an older stellar population with lower rates of ongoing star formation. Fainter, bluer regions extend from the core, indicating the presence of younger stars or regions of recent star formation, although not prominently so. A faint disk-like structure could be suggested by the elongated morphology, but there are no apparent spiral arm structures. Overall the galaxy appears relatively undisturbed.
