The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a moderate degree of ellipticity, appearing somewhat elongated in shape. The color profile suggests a dominant population of older stars, evidenced by a redder hue. There is little evidence of distinct spiral arms or significant dust lanes, supporting the smooth morphology classification. The galaxy appears to lack a prominent, actively star-forming nucleus based on the relatively uniform color distribution. The overall structure suggests a system that has largely exhausted its supply of gas, resulting in a lower star formation rate. There may be some minor disturbances in the outer regions of the galaxy, hinting at potential past interactions or minor merger events.
