This galaxy exhibits a predominantly smooth morphology, with an elliptical or lenticular shape. There's a slight elongation evident in its structure, deviating from a perfectly circular form. A color gradient is visible, with a central region displaying a warmer, yellower hue, potentially indicating a higher concentration of older stellar populations. This fades to a cooler, redder color in the outer regions, potentially suggesting a decrease in stellar density or presence of a slightly younger stellar population. No distinct spiral arms or features are readily apparent; the light distribution appears relatively uniform. The absence of prominent dust lanes or star-forming regions further supports its classification as a more evolved, passively evolving system, with an estimated mass range of 10^10.5 to 10^10.6 solar masses. There are subtle indications of a minor gravitational disturbance or interaction, possibly a slight asymmetry in the outer halo's isophotes; however, more data is required to confirm this.
