The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white luminosity, suggestive of an older stellar population dominating the central region. There is little evidence of distinct spiral arms or prominent dust lanes. The color profile shows a generally redder hue, indicating that the object is likely a more mature system. No tidal tails or other clear signs of recent major merger events are apparent from visual inspection of the image, although subtle asymmetries could be present. Given the apparent smoothness and lack of significant features, it is probable that this galaxy is an elliptical galaxy undergoing relatively low levels of current star formation.
