The galaxy presents as a fairly elliptical, well-defined structure with a smooth morphology. There is a concentration of light towards the center, suggesting a prominent galactic bulge. The galaxy exhibits a yellow-orange hue, potentially indicative of an older stellar population and a relatively low rate of ongoing star formation. No distinct spiral arm structure or prominent dust lanes are visible in this image, further supporting the classification as a relatively featureless elliptical galaxy. The light distribution is largely uniform, with no significant signs of tidal disturbances, major mergers, or other morphological peculiarities. The galaxy appears round, with only a slight elongation. Based on the color and morphology, this object is likely a mature galaxy with a significant stellar mass.
