This galaxy presents as a moderately luminous object, exhibiting a roughly elliptical morphology. The luminosity increases towards the center. A very slight asymmetry is evident, possibly indicating a minor gravitational interaction or internal disturbance. The galaxy's color profile suggests a slightly redder hue, potentially indicating an older stellar population, or the presence of dust. No prominent spiral arms or bar structures are discernible. There may be a hint of a disk. Based on the presence of minor disturbances, the galaxy appears to not be undergoing major mergers, but may have merged in the past.
