The galaxy presents an elliptical morphology with a smooth, concentrated central bulge exhibiting a yellow-orange hue. The outer regions of the galaxy appear more diffuse and less chromatic, suggesting an older stellar population compared to the core. The shape is elongated, deviating from a perfect circle, with an axial ratio indicating a possible classification between E4 and E6 on the Hubble sequence. There is no clear evidence of spiral arms, dust lanes, or ongoing major merging activity. Minor disturbances are not ruled out. The galaxy exhibits a high degree of central concentration, with light intensity decreasing smoothly from the center outwards. The overall appearance suggests a relatively passive system, likely with a low rate of star formation.
