The galaxy appears as a central, concentrated, relatively smooth object. It exhibits a faint, diffuse, and elongated morphology. A subtle color gradient can be observed, where the core seems to be primarily blue-white, possibly indicating a population of younger, hotter stars. The outer regions have a somewhat reddish-brown hue, which could indicate older stellar populations or dust obscuration. There is no clear evidence of spiral arms, bars, or other distinct morphological features. The overall impression is that of a relatively quiescent system, without significant ongoing major star formation activity or recent merger events.
