The galaxy presents an elliptical morphology, appearing largely smooth in structure without readily discernible spiral arms or a prominent disk. It exhibits a central, luminous bulge that fades gradually into the outer regions. The colour profile shows a concentration of bluer hues towards the central regions, suggesting a population of younger, hotter stars or active star formation within the core. The overall structure implies a system with a substantial stellar mass, showing low star formation activity but a higher mass range. There's a very slight hint of possible minor disturbance, and its is cigar-shaped, but its form is overwhelmingly smooth. The majority of light appears to be concentrated toward the center, with a decreasing intensity gradient toward the edges, indicative of an older stellar population. 
