The galaxy presents a largely smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The primary color of the galaxy is a yellow-white hue, suggesting an older stellar population dominating the overall light emission. A prominent dust lane is observed bisecting the galaxy’s center along its major axis, obscuring a portion of the bulge light. The galaxy shows no readily apparent spiral arm structure or significant tidal features, suggesting a relatively undisturbed evolutionary history. It has an estimated effective radius of approximately 6 kpc. A low level of ongoing star formation activity may be present.
