The galaxy presents as a somewhat amorphous structure, with a dominant central bulge that appears nearly spherical. The light distribution is relatively smooth, with a significant concentration of luminosity toward the nucleus, but also a noticeable, yet less pronounced, distribution away from this central region. The overall color of the galaxy shows hints of younger, bluer stars in the outer regions, indicative of ongoing or recent star formation, while the core appears more yellowish-red, which may imply an older stellar population residing within the bulge. There is a hint of possible interaction or disturbance, evidenced by the slight elongation and asymmetrical shape of the main body. It seems like a possible minor interaction.
