The galaxy presents a predominantly elliptical morphology, appearing largely smooth in structure. A subtle, blue-tinged disk-like feature is observed extending perpendicularly from the central bulge, possibly indicative of recent or ongoing star formation within a flattened distribution of gas and dust. The central bulge exhibits a reddish hue, suggesting a population of older, redder stars. The overall shape suggests a galaxy transitioning from a spiral to an elliptical form, or possibly an elliptical galaxy with some residual star formation activity. There are no prominent tidal features or morphological disturbances visible, suggesting it is a relatively isolated system, although minor disturbances cannot be ruled out. The relatively compact size indicates it may be a dwarf galaxy or a more distant, larger galaxy where details are not resolvable at the present image scale.
