The galaxy presents as a centrally concentrated, smooth structure, exhibiting a generally elliptical morphology. It appears relatively featureless with no prominent spiral arms or distinct dust lanes visible in the image. The light profile seems to decline smoothly from the core, suggesting a relatively old stellar population and a lack of significant ongoing star formation. There is no obvious indication of a recent or ongoing major merger, but a minor disturbance cannot be ruled out based on this image alone. The overall color is consistent with a redder galaxy, further supporting the interpretation of an older stellar population with a low specific star formation rate. The galaxy's apparent roundness suggests it may be closer to an E0 type elliptical.
