The galaxy presents a generally smooth and rounded morphology, exhibiting characteristics more consistent with an elliptical galaxy than a spiral. The central region displays a concentrated brightness, indicative of a significant stellar population and potential active galactic nucleus activity. The outer regions fade gradually, lacking defined spiral arms or distinct features. There's minimal evidence of significant tidal disturbances or ongoing major merger activity, suggesting the galaxy is relatively undisturbed. Some subtle, diffuse features can be noted, but they do not dominate the overall appearance. The color profile indicates a potentially older stellar population, biased towards the redder end of the spectrum. This galaxy is estimated to be roughly 5.5 kpc across.
