The galaxy presents as a relatively smooth and centralized object. Its overall form appears elliptical, tending toward a flattened shape rather than perfectly spherical. There is no clear evidence of spiral arm structures or a well-defined disk. A slight color gradient is present, with the core exhibiting a somewhat bluer or possibly pinker hue. This might indicate a population of younger, hotter stars in the central region, but it is also possible that the central region exhibits increased dust or gas, affecting the color. The outer regions of the galaxy appear less luminous and have a redder color, suggesting an older stellar population. There are possible irregularities or minor disturbances present in the morphology, however, the galaxy's overall structure gives the appearance of a single, somewhat isolated object. There are no indications of a major merger event currently underway, though past interactions cannot be ruled out. The outer edges of the galaxy are diffuse and fade gradually into the background.