The galaxy presents a generally smooth appearance, with a central, brighter region likely indicating a bulge component. It appears to be an intermediate disk galaxy with an estimated effective radius of approximately 5 kpc. There is some indication of a possible disk or arm structures extending outward from the central bulge, but these features appear somewhat disturbed and asymmetrical, implying it may have undergone a minor interaction. The dominant color is a bluish-white, suggesting the presence of a moderate population of relatively young, hot stars. Overall, the galaxy does not exhibit signs of major star formation or major merger activity.
