The galaxy presents a generally smooth morphology, exhibiting a mostly elliptical shape. The light is primarily concentrated in the center, appearing as a bright, concentrated central bulge, indicating a high stellar density in that region. The galaxy appears moderately luminous, especially in redder wavelengths, which suggests a population dominated by older, redder stars. There appears to be little to no evidence of spiral arms or a well-defined disk structure. Additionally, there is no obvious dust lane. Overall, the galaxy seems to be relatively undisturbed, without major tidal features or signs of an ongoing merger.
