The galaxy presents as a relatively smooth, elliptical structure with a central bulge. The galaxy exhibits a yellow-orange hue, suggesting a population of older stars and a lack of significant ongoing star formation. The overall shape is somewhat rounded, showing minimal signs of spiral arms or a prominent disk structure. There is a slight suggestion of a tidal disturbance or possible minor interaction with a smaller companion galaxy to the upper right, based on subtle visual irregularities in the light distribution. The galaxy appears moderately massive, likely around 10^11 solar masses, and exhibits a low rate of star formation.
