The galaxy presents a generally smooth morphology, with a central bulge that dominates the overall luminosity. The shape is neither perfectly circular nor highly elongated, appearing somewhat in between. The galaxy displays a gradient in color, with the central region exhibiting a yellower hue, suggestive of an older stellar population. Moving outwards from the center, the galaxy gradually fades, showing a subtle transition towards bluer tones, potentially indicating the presence of younger, hotter stars. There is a faint, redder patch at one end, which could potentially indicate the presence of an area of dust or recent star formation. While the main body of the galaxy appears relatively undisturbed, there is a very slight asymmetry noticeable that warrants further inspection.
