The galaxy appears as a concentrated, luminous object with an overall elliptical morphology. It exhibits a smooth, largely featureless structure, lacking any prominent spiral arms or bar-like formations. The central region displays the highest surface brightness, gradually decreasing towards the outer edges. The galaxy's color profile suggests a relatively older stellar population, with a dominant yellowish-orange hue. Faint blue tinges can be seen suggesting some star formation present within. There are some signs of minor disturbances, but on the whole the galaxy appears relatively isolated. The high degree of roundness indicates a minimal degree of inclination relative to the observer's line of sight.
