The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. It appears nearly circular in projection, with a lack of discernible spiral arms or a distinct disk structure. The color profile indicates an older stellar population, as suggested by the redder hue. There is no evidence of significant dust lanes or active star formation regions. Faint tidal features might be present, suggesting a past or ongoing interaction with another galaxy, though these features are ambiguous and require further investigation. There is a slight elongation of the halo, indicating that it may not be perfectly spherical. The image's angular resolution limits further detailed morphological classification.
