The galaxy presents as an elliptical system exhibiting a concentrated central bulge. The light distribution is generally smooth with an apparent lack of resolved features. The galaxy's overall shape is elongated, demonstrating a degree of asymmetry. It does appear there is some sort of tidal disturbance or merger occurring with a secondary object. The color profile tends towards warmer tones, suggesting an older stellar population within the bulge. Some star formation is likely present. The central bulge dominates the overall luminosity, but appears slightly offset. There is evidence of a red component on one side, which might indicate a dust lane or region of obscured star formation.
