The galaxy presents a largely smooth, rounded morphology with a concentrated central bulge. Color gradients are observable; the central region exhibits a yellowish hue, possibly indicative of an older stellar population. Progressing outward from the core, a subtle shift towards bluer colors is apparent, suggesting the presence of younger, star-forming regions in the outer regions. There is no clear evidence of spiral arm structure or a well-defined disk component. The overall structure appears relatively undisturbed, lacking signs of major merger activity, although some subtle irregularities in the outer regions may indicate minor gravitational interactions. The galaxy is estimated to be a significant mass, with a moderate rate of star formation.
