The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile towards the center. The galaxy's core appears yellowish-orange, suggesting an older stellar population. A slight bluer hue is detected in the outer regions, hinting at the presence of younger, hotter stars, although the rate of star formation appears relatively low. The axial ratio indicates the galaxy is somewhat elongated but not severely so, and it doesn't appear to be undergoing any major mergers or significant tidal disturbances, though a minor disturbance cannot be ruled out. The estimated physical size of the galaxy is moderate.
