The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its core exhibits a bright, concentrated luminosity, indicative of a high stellar density. There is a gradual decrease in brightness moving from the center outwards, suggesting a smooth stellar distribution without prominent spiral arm structures or significant dust lane obscuration. The overall shape tends toward a slightly elongated spheroid, though it is largely featureless. Faint blue-tinged regions may suggest some ongoing, though likely subdued, star formation activity. The galaxy appears relatively isolated, showing no signs of tidal distortion or interaction with other nearby galaxies.
