The galaxy presents a somewhat elongated, elliptical morphology. It exhibits a concentrated central bulge that is bright yellow, suggesting an older stellar population. The galaxy appears largely featureless, showing a smooth luminosity profile without discernible spiral arms or dust lanes. A faint, blue-ish glow is present on the left side of the galaxy, which might indicate the presence of younger stars and active star formation regions, though it is quite dim. There are no apparent signs of a major merger, but some minor disturbances may be present in its overall structure. The light distribution suggests a galaxy that is in an intermediate state between a disk-dominated and a spheroid-dominated system. Overall, the galaxy appears relatively quiescent with low ongoing star formation.
