The galaxy appears as a centrally concentrated object with a relatively smooth, amorphous structure. The light distribution suggests a spheroidal morphology, lacking any obvious spiral arms or a well-defined disk. There is a bright central region that could indicate the presence of an active galactic nucleus or a dense concentration of stars. The overall color is consistent with an older stellar population, possibly with some on-going star formation. A faint, diffuse halo extends outward from the central region, gradually fading into the background. The galaxy exhibits only slight asymmetries, hinting at a dynamically relaxed system or possibly a minor disturbance event in its past.
