The galaxy presents as a relatively smooth, elliptical morphology. It displays a concentrated central bulge, diminishing in intensity outwards. The overall color profile appears to be a mix of light, trending towards yellow and red hues in the core, which may imply an older stellar population. There is a slight hint of blue on one side of the disk that may indicate a small amount of star formation. The galaxy does not appear to show any major disturbances or signs of an ongoing merger event. Its elliptical shape suggests that it may be a product of previous galactic mergers, but it presents as a well-formed, stable structure.
