The galaxy presents an overall elliptical morphology, though not perfectly symmetrical. It exhibits a diffuse, extended halo, with the central region appearing brighter and more concentrated. Within the central area, there is a notable concentration of bluer light, suggesting the presence of a population of younger, hotter stars or perhaps ongoing star formation activity in that locale. The bulk of the galaxy shows a redder hue, which indicates an older stellar population dominating the overall light output. There are indications of minor disturbances in the galaxy's structure, possibly hinting at past or ongoing interactions with smaller companions. There is no prominent disk structure visible, and overall, the galaxy appears relatively smooth with minimal signs of spiral arms or significant dust lanes. 
