The galaxy presents as a centrally concentrated, smooth structure. There is a noticeable radial color gradient, transitioning from a warmer, yellower hue in the central region to cooler, bluer tones in the outer regions. The isophotes appear mostly regular, suggesting minimal recent merger activity or strong tidal interactions. Its shape is approximately round and the absence of well-defined spiral arms or a prominent disk indicates a relatively featureless morphology. There are only minor disturbances within the galaxy.
