The galaxy presents as a relatively smooth, elongated structure, suggesting an elliptical morphology, possibly of type E4-E7. The central region exhibits a concentrated luminosity. There is a distinct color gradient, transitioning from a yellow-orange core to a redder outer halo. This may indicate an older stellar population dominating the central bulge, with potentially ongoing, albeit low, star formation in the outer regions or a dust lane attenuating blue light. There is no clear evidence of spiral arms or a well-defined disk structure. Faint disturbances may be present, but they are not pronounced, so it is likely it is not currently undergoing a major merging event.
