The galaxy presents an elliptical morphology, though not perfectly symmetrical. The central bulge appears prominent and exhibits a yellow-orange hue, indicating a population of older stars. Fainter, bluer regions are also visible, particularly in what could be considered the disk area, suggesting some ongoing star formation despite the dominant presence of older stellar populations. There may be a slight disturbance in the galaxy's overall structure, perhaps indicative of a past or ongoing interaction, but the system is currently not in the midst of a major merging event. The light profile shows a degree of smoothness with some features. There is a brighter concentration of light at its center. The general color of the object is yellow.