The galaxy appears to be a single, somewhat spheroidal structure with a smooth, diffuse light distribution. The central region exhibits a significantly higher concentration of light, appearing as a bright, yellowish core. Fainter, reddish extensions surround this core, suggesting the presence of older stellar populations. There is little evidence of distinct spiral arms or a well-defined disk, and the morphology appears largely undisturbed, with no major signs of ongoing merger activity or tidal distortions. The galaxy appears moderately massive and possesses a moderate rate of star formation.
