The galaxy presents a predominantly smooth, elliptical morphology. Its shape is generally rounded but shows some elongation, tending towards a cigar-like appearance. The central region exhibits a concentrated, bright core that gradually diffuses outwards. There is a color gradient observable, where the central core exhibits a yellowish-white hue, transitioning to a redder tone at the outer edges. The overall structure doesn't reveal any significant signs of ongoing merging events or major disturbances; however, there might be minor irregularities in the outer regions that warrant further investigation. Given the smooth appearance, redder hue, and absence of prominent spiral arms, the galaxy appears to be a mature system with a relatively low star formation rate.
