The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentration of light, appearing as a bright, yellowish core. Moving outward from the core, the light intensity decreases gradually, forming a more diffuse halo. While there are some subtle color variations, overall the galaxy appears relatively homogenous in color distribution, with a tendency towards redder hues in the central regions. There is no discernible spiral arm structure or significant dust lane obscuration evident in the image. The galaxy appears generally undisturbed, without prominent tidal tails or other signs of recent merger activity, though some faint asymmetry could indicate minor gravitational interactions. The apparent size and shape suggest this is likely an early-type galaxy viewed at some distance.
