The galaxy exhibits a generally smooth morphology, with a notable absence of well-defined spiral arms or a prominent central bar structure. The light distribution indicates an elliptical-like shape, though not perfectly spherical, appearing somewhat elongated. The galaxy demonstrates a color gradient, with the central region displaying a yellowish-orange hue, suggesting an older stellar population. Progressing outwards from the core, the color shifts towards a bluer tint, implying the presence of younger, hotter stars in the outer regions. There is a slight indication of some mild disturbance or asymmetry in the galaxy's structure. No strong tidal features are evident, such as extended tails or bridges that would indicate recent major merger activity. Overall, the galaxy appears to be a relatively isolated system, with a moderately high mass and a moderate rate of star formation.
