The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a high degree of roundness. There is a slight elongation or disturbance in the morphology, but overall, the disk structure, if any, is not clearly dominant. The light distribution appears concentrated, with a brighter central region that fades into a more diffuse halo. The color profile indicates a moderate level of on-going star formation with hints of activity in the blue wavelengths. No strong spiral arm structures are apparent. There appears to be a possible companion galaxy in the vicinity; however, tidal disturbances or clear signs of a recent merger are not clearly observed. The overall appearance suggests a galaxy with moderate luminosity and a relatively stable configuration.
