The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The light profile suggests a relatively high degree of central concentration. The overall shape tends toward circularity, with minimal observed elongation. There is a suggestion of some structural irregularity, as the object isn't perfectly smooth and round. The light from the galaxy has a yellowish tint, suggesting it is not actively forming many new stars. There is no apparent interaction or merging activity with other galaxies.
