This galaxy exhibits a generally smooth morphology, appearing largely elliptical in shape. There is some evidence of possible disturbances within the galactic structure. While the central region appears relatively uniform in color, there is a subtle blue tint to the outer edges which may signify more recent star forming events.

The galaxy is moderately compact, lacking prominent extended features. The overall appearance is more rounded than elongated, suggesting a classification leaning towards elliptical rather than a highly flattened disk galaxy viewed edge-on. There may be some evidence of a minor tidal interaction, but it is difficult to say for sure without further investigation. The color distribution suggests a relatively mature stellar population, with a moderate amount of ongoing star formation.
