The galaxy presents a largely smooth, elliptical morphology. Its light profile appears highly concentrated toward the center, suggesting a relatively old stellar population. The galaxy exhibits a yellow-red hue, possibly indicating a lack of significant ongoing star formation. The galaxy appears to be primarily spheroidal, with little evidence of a disk-like structure. There might be a slight irregularity present but no major disturbances or merging features are visible. The shape is mostly round.
