The galaxy presents a generally smooth morphology. The dominant color appears to be a yellow-orange hue, concentrated towards the central region, suggesting an older stellar population in the core. The isophotes suggest a shape that is neither perfectly round nor significantly elongated, existing somewhere in between. There might be minor disturbances in the outer regions, possibly indicative of past or ongoing interactions. Overall, the galaxy appears relatively undisturbed, showing a lack of major merging events in its recent history.
