The galaxy presents a somewhat elliptical morphology, appearing neither perfectly spherical nor highly elongated. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus or bulge. Surrounding this bright core, a fainter, diffuse disk is observed. The color profile appears to show a yellow-ish center, possibly indicative of an older stellar population, transitioning to bluish hues in the outer disk, potentially due to ongoing star formation or a younger stellar population. There is a very slight suggestion of asymmetry or minor disturbances in the morphology, potentially hinting at past interactions, but it seems largely undisturbed. The disk shows some granularity but not large spiral arm structures. Overall the galaxy seems to be transitioning away from blue star formation, likely a disk galaxy. 
