The galaxy presents a largely smooth, elliptical morphology. It appears moderately bright and somewhat compact, exhibiting a relatively featureless structure without prominent spiral arms or a well-defined disk. The light distribution is concentrated toward the center, with a gradual fading toward the edges, suggesting a spheroidal shape.

The galaxy exhibits a color gradient. The central region appears slightly more blue/white, possibly indicating a population of younger, hotter stars, while the outer regions display a redder hue suggesting an older, redder stellar population.

There is no apparent evidence of strong tidal disturbances, major ongoing mergers, or significant star formation regions. Its overall appearance suggests that it is a relatively undisturbed system with an older stellar population. The galaxy is neither perfectly round nor elongated in its appearance. 
