The galaxy presents a generally smooth morphology, with a central, concentrated bulge exhibiting a yellow-white hue. There is a fainter, more diffuse disk component visible, displaying blueish tinges on one side of the galaxy, suggesting the presence of younger stellar populations or ongoing star formation in this region. The opposite side of the galaxy fades into the background with similar yellowish hues like the bulge. There appears to be a slight asymmetry in the galaxy's overall form, possibly indicating a minor gravitational disturbance or interaction. No distinct spiral arm structures are discernible.
