The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The central bulge exhibits a concentrated luminosity, grading outward into a more diffuse halo. The galaxy displays a yellowish-white color, possibly indicative of an older stellar population dominating the light output. There is a subtle color gradient across the galaxy, with the central region appearing slightly redder than the outer regions, possibly due to increased dust obscuration or a higher concentration of older, redder stars in the core. No distinct spiral arms or prominent dust lanes are discernible. The overall structure suggests a relatively evolved system, potentially an elliptical galaxy, without significant ongoing star formation evident in this image.
