The galaxy presents as a smooth, elliptical-like structure. It exhibits a bright central bulge, possibly indicative of an older stellar population, gradually fading into a less dense halo. There is a slight elongation, suggesting a deviation from a perfectly spherical shape. The color profile appears to be relatively uniform with a yellow hue, implying a lack of significant ongoing star formation. There is no discernable dust lane or spiral arm structure visible in the image. The galaxy appears undisturbed, showing no obvious signs of recent merger events. The outer edges fade gradually, suggesting a smooth transition into the intergalactic medium.
