The galaxy presents a largely smooth and rounded morphology. The central region exhibits a concentrated luminosity, appearing brighter and more diffuse than the outer regions. A subtle color gradient is observed, shifting from a bluer hue in the inner region to a slightly redder tone towards the outer edges. There is minimal evidence of significant spiral arm structure or prominent dust lanes. The overall appearance suggests a relatively evolved system, consistent with a galaxy undergoing limited current star formation. There is a possible indication of a minor tidal disturbance or interaction occurring within the galaxy, although this could potentially be an artifact of the image.
