The galaxy presents as a compact, moderately bright object with a discernible central concentration. Its morphology appears somewhat smooth, with a slight elongation but not exhibiting a strong disk structure. The color profile suggests the presence of both older stellar populations and a component of ongoing star formation, indicated by the blue hues particularly in the central regions. There is no clear evidence of spiral arms or a bar structure. Additionally, there are no obvious signs of major mergers or tidal disturbances in this image, though minor disturbances cannot be ruled out. The object is quite compact.
