The galaxy presents as a relatively compact object with a dominant smooth, centrally concentrated morphology. The light profile suggests a high degree of sphericity, appearing nearly round in shape. However, there is evidence of some subtle asymmetry, with a slight irregularity on one side, possibly indicating a minor disturbance or interaction. 

The galaxy's color is primarily blue-white, indicative of a population of relatively young, hot stars. However, a faint redder patch suggests an older stellar population, potentially within a bulge component or a region of dust obscuration. Overall, the galaxy displays relatively low levels of ongoing star formation activity.

